First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results

Abstract

We present full sky microwave maps in five bands (23 to 94 GHz) from the WMAP first year sky survey. Calibration errors are <0.5% and the low systematic error level is well specified. The 2<l<900 anisotropy power spectrum is cosmic variance limited for l<354 with a signal-to-noise ratio >1 per mode to l=658. The temperature-polarization cross-power spectrum reveals both acoustic features and a large angle correlation from reionization. The optical depth of reionization is 0.17 +/- 0.04, which implies a reionization epoch of 180+220-80 Myr (95% CL) after the Big Bang at a redshift of 20+10-9 (95% CL) for a range of ionization scenarios. This early reionization is incompatible with the presence of a significant warm dark matter density. The age of the best-fit universe is 13.7 +/- 0.2 Gyr old. Decoupling was 379+8-7 kyr after the Big Bang at a redshift of 1089 +/- 1. The thickness of the decoupling surface was dz=195 +/- 2. The matter density is Omega_m h^2 = 0.135 +0.008 -0.009, the baryon density is Omega_b h^2 = 0.0224 +/- 0.0009, and the total mass-energy of the universe is Omega_tot = 1.02 +/- 0.02. The spectral index of scalar fluctuations is fit as n_s = 0.93 +/- 0.03 at wavenumber k_0 = 0.05 Mpc^-1, with a running index slope of dn_s/d ln k = -0.031 +0.016 -0.018 in the best-fit model. This flat universe model is composed of 4.4% baryons, 22% dark matter and 73% dark energy. The dark energy equation of state is limited to w<-0.78 (95% CL). Inflation theory is supported with n_s~1, Omega_tot~1, Gaussian random phases of the CMB anisotropy, and superhorizon fluctuations. An admixture of isocurvature modes does not improve the fit. The tensor-to-scalar ratio is r(k_0=0.002 Mpc^-1)<0.90 (95% CL).

Replaced with version accepted by ApJ. One of thirteen companion papers on first-year WMAP results; 43 pages, 17 figures; a version with higher quality graphics is at http://lambda.gsfc.nasa.gov/

References in corpus (24)

• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Emission
• Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Tests of Gaussianity
• Detection of Polarization in the Cosmic Microwave Background using DASI
• The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Parameter Estimation Methodology
• The Microwave Anisotropy Probe (MAP) Mission
• A Full-Sky H-alpha Template for Microwave Foreground Prediction
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks
• The Universe Was Reionized Twice
• The Anisotropy of the Microwave Background to l = 3500: Mosaic Observations with the Cosmic Background Imager
• The White Dwarf Cooling Sequence of the Globular Cluster Messier 4
• The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing Methods and Systematic Errors Limits
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles and Window Functions
• Design, Implementation and Testing of the MAP Radiometers
• The CMB power spectrum out to l=1400 measured by the VSA
• The Optical Design and Characterization of the Microwave Anisotropy Probe
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: On-Orbit Radiometer Characterization
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Signal Contamination from Sidelobe Pickup
• The MAP Satellite Feed Horns

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• Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Polarization
• The Dipole Anisotropy of the 2 Micron All-Sky Redshift Survey
• The Cosmic Web: Geometric Analysis
• Accelerated expansion from a non-minimal gravitational coupling to matter
• Two Field Matter Bounce Cosmology
• A measurement of the Hubble constant from Type II supernovae
• Mimicking Dark Energy with Lemaitre-Tolman-Bondi Models: Weak Central Singularities and Critical Points
• Heavy Wino-like Neutralino Dark Matter Annihilation into Antiparticles
• Dark Matter Relic Abundance and Scalar-Tensor Dark Energy
• Constraining Running Non-Gaussianity
• Bayesian analysis of sparse anisotropic universe models and application to the 5-yr WMAP data
• Rotating black hole in extended Chern-Simons modified gravity
• Cosmological parameter constraints from SDSS luminous red galaxies: a new treatment of large-scale clustering
• Gravitino Dark Matter in the CMSSM and Implications for Leptogenesis and the LHC
• Accelerating cosmologies from M/String theory compactifications
• Cosmology of hybrid metric-Palatini f(X)-gravity
• Big Crunch Avoidance in k = 1 Semi-Classical Loop Quantum Cosmology
• Phenomenological Tests of Supersymmetric A_4 Family Symmetry Model of Neutrino Mass
• Constraining slow-roll inflation with WMAP and 2dF
• Gravitational Theory, Galaxy Rotation Curves and Cosmology without Dark Matter
• Primordial Non-Gaussianity and Analytical Formula for Minkowski Functionals of the Cosmic Microwave Background and Large-scale Structure
• Detection of anomalous microwave emission in the Perseus molecular cloud with the COSMOSOMAS experiment
• Energy conditions in modified Gauss-Bonnet gravity
• An alternative to the cosmological 'concordance model'
• High-precision predictions for the acoustic scale in the non-linear regime
• Shortcomings in the Understanding of Why Cosmological Perturbations Look Classical
• Suppression and Spatial Variation of Early Galaxies and Minihalos
• The nearly Newtonian regime in Non-Linear Theories of Gravity
• CMB polarization features from inflation versus reionization
• Some Bianchi Type Cosmological Models in f(R) Gravity
• Efficient Bayesian inference for multimodal problems in cosmology
• Planck 2013 results. XXVI. Background geometry and topology of the Universe
• The Cauchy problem of scalar-tensor theories of gravity
• Measurements of H(z) and D_A(z) from the Two-Dimensional Two-Point Correlation Function of Sloan Digital Sky Survey Luminous Red Galaxies
• Physical non-equivalence of the Jordan and Einstein frames
• Chandra and XMM-Newton Observations of RDCS1252.9-2927, A Massive Cluster at z=1.24
• The Lithium Content of the Galactic Halo Stars
• The power spectrum of the flux distribution in the Lyman-alpha forest of a Large sample of UVES QSO Absorption Spectra (LUQAS)
• Present status of primordial nucleosynthesis after WMAP: results from a new BBN code
• CMB component separation by parameter estimation
• Constraining invisible neutrino decays with the cosmic microwave background
• Multi-Dimensional mSUGRA Likelihood Maps
• Observables sensitive to absolute neutrino masses: Constraints and correlations from world neutrino data
• Measurement of the gravitational potential evolution from the cross-correlation between WMAP and the APM Galaxy survey
• The Parsec-Scale Structure and Jet Motions of the TeV Blazars 1ES 1959+650, PKS 2155-304, and 1ES 2344+514
• The Axis of Evil revisited
• Exact Solutions of Bianchi Types $I$ and $V$ Spacetimes in $f(R)$ Theory of Gravity
• Brans-Dicke Scalar Field as a Chameleon
• Cross-correlation of the CMB and radio galaxies in real, harmonic and wavelet spaces: detection of the integrated Sachs-Wolfe effect and dark energy constraints
• Attractor Solutions in f(T) Cosmology
• The radio structure of radio-quiet quasars
• The Complex Cooling Core of Abell 2029: Radio and X-ray Interactions
• The hot subdwarf B + white dwarf binary KPD 1930+2752 - a Supernova Type Ia progenitor candidate
• The minimal model of fermionic dark matter
• Phantom Cosmologies
• Analysis of First LIGO Science Data for Stochastic Gravitational Waves
• Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data
• New Observational $H(z)$ Data from Full-Spectrum Fitting of Cosmic Chronometers in the LEGA-C Survey
• Phantom-like GCG and the constraints of its parameters via cosmological dynamics
• Galaxy groups in the low-redshift Universe
• New asymptotically flat phantom wormhole solutions
• Effects of Unstable Particles on Light-Element Abundances: Lithium versus Deuterium and He3
• Big bang nucleosynthesis constraints on scalar-tensor theories of gravity
• Bianchi Type-$V$ cosmology in $f(R,T)$ gravity with $\Lambda (T)$
• Rethinking CMB foregrounds: systematic extension of foreground parameterizations
• Scaling of Multi-Tension Cosmic Superstring Networks
• Cosmological acceleration, varying couplings, and Lorentz breaking
• Instrument, Method, Brightness and Polarization Maps from the 2003 flight of BOOMERanG
• Mixed inflaton and curvaton perturbations
• Silk damping at a redshift of a billion: a new limit on small-scale adiabatic perturbations
• Exact solution of scalar field cosmology with exponential potentials and transient acceleration
• Induced two-photon decay of the 2s level and the rate of cosmological hydrogen recombination
• Which spectral distortions does $\Lambda$CDM actually predict?
• Cosmic shear statistics in the Suprime-Cam 2.1 sq deg field: Constraints on Omega_m and sigma_8
• Observational $H(z)$ Data and Cosmological Models
• The Cosmological Dynamics of Interacting Holographic Dark Energy Model
• Massive Coronae of Galaxies
• Constraints on a Bianchi type I spacetime extension of the standard $\Lambda$CDM model
• Quintom model with O($N$) symmetry
• Clustering of quasars in SDSS-IV eBOSS : study of potential systematics and bias determination
• CMB multipole measurements in the presence of foregrounds
• X-ray Temperatures for the EMSS High Redshift Cluster Sample: Constraints on Cosmology and the Dark Energy Equation of State
• Tachyon inflation: tests and comparison with single scalar field inflation
• Gluino Decays in Split Supersymmetry
• On the Decoherence of Primordial Fluctuations During Inflation
• Observing Brane Inflation
• The Emergence of the Thick Disk in a CDM Universe II: Colors and Abundance Patterns
• Is the Universe odd?
• Fast Estimator of Primordial Non-Gaussianity from Temperature and Polarization Anisotropies in the Cosmic Microwave Background
• Structure formation with strongly interacting neutrinos - implications for the cosmological neutrino mass bound
• Naturalness Priors and Fits to the Constrained Minimal Supersymmetric Standard Model
• Integrated Sachs-Wolfe effect in Cross-Correlation: The Observer's Manual
• Cosmological Signatures of Interacting Neutrinos
• A Catalog of Local E+A(post-starburst) Galaxies selected from the Sloan Digital Sky Survey Data Release 5
• A History of HI Stripping in Virgo: A Phase-space View of VIVA Galaxies
• Cosmo-dynamics and dark energy with non-linear equation of state: a quadratic model
• Ionizing radiation fluctuations and large-scale structure in the Lyman-alpha forest
• Stability of the Einstein static universe in modified Gauss-Bonnet gravity
• WMAP constraints on SUGRA models with non-universal gaugino masses and prospects for direct detection
• Big Bang Nucleosynthesis with a New Neutron Lifetime
• Probing the equation of state of the early universe with a space laser interferometer
• The Formation of the First Stars in the Universe
• An updated Gamma Ray Bursts Hubble diagram
• Experimental Tests of General Relativity: Recent Progress and Future Directions
• Noether Symmetry Approach in f(R) Tachyon Model
• Can superhorizon cosmological perturbations explain the acceleration of the universe?
• Dark energy models with variable equation of state parameter
• CMB temperature and polarisation pseudo-Cl estimators and covariances
• Cosmological quantum entanglement
• Correlating the CMB with Luminous Red Galaxies : The Integrated Sachs-Wolfe Effect
• The Hot and Cold Spots in the WMAP Data are Not Hot and Cold Enough
• The KBC void and Hubble tension contradict $\Lambda$CDM on a Gpc scale $-$ Milgromian dynamics as a possible solution
• Interacting agegraphic dark energy models in non-flat universe
• Sneutrino Inflation in the Light of WMAP: Reheating, Leptogenesis and Flavour-Violating Lepton Decays
• Model-Independent Reconstruction of the Primordial Power Spectrum from WMAP Data
• Considerations in optimizing CMB polarization experiments to constrain inflationary physics
• On the reheating stage after inflation
• Phantom Cosmic Dynamics: Tracking Attractor and Cosmic Doomsday
• Renormalization-group running cosmologies - a scale-setting procedure
• Observing Dark Energy Dynamics with Supernova, Microwave Background and Galaxy Clustering
• Testing the Void against Cosmological data: fitting CMB, BAO, SN and H0
• Phantom cosmology with general potentials
• Measuring Dark Energy Clustering with CMB-Galaxy Correlations
• Age Problem in the Holographic Dark Energy Model
• Gravitational Leptogenesis and Its Signatures in CMB
• Mismatch between X-ray and emission-weighted temperatures in galaxy clusters: cosmological implications
• Inflation from Superstring/M Theory Compactification with Higher Order Corrections I
• Quintessence reconstruction of the new agegraphic dark energy model
• The Atacama Cosmology Telescope: DR5 maps of 18,000 square degrees of the microwave sky from ACT 2008-2018 data
• Lorentz Violating Inflation
• Formation of the Black Holes in the Highest Redshift Quasars
• Higher Criticism Statistic: Detecting and Identifying Non-Gaussianity in the WMAP First Year Data
• WMAPing the Universe: Supersymmetry, Dark Matter, Dark Energy, Proton Decay and Collider Physics
• Observational constraints on holographic dark energy with varying gravitational constant
• The fate of four dimensions
• Upper Limits on a Stochastic Background of Gravitational Waves
• Some Issues Concerning Holographic Dark Energy
• Lines in the Cosmic Microwave Background Spectrum from the Epoch of Cosmological Hydrogen Recombination
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: the low redshift sample
• Feedback in the local LBG Analog Haro 11 as probed by far-UV and X-ray observations
• Cosmological parameters from strong gravitational lensing and stellar dynamics in elliptical galaxies
• Cosmology with High-redshift Galaxy Survey: Neutrino Mass and Inflation
• Cosmological variation of deuteron binding energy, strong interaction and quark masses from big bang nucleosynthesis
• Exact reconstruction with directional wavelets on the sphere
• The impacts of dark matter particle annihilation on recombination and the anisotropies of the cosmic microwave background
• Dark Matter in the Milky Way's Dwarf Spheroidal Satellites
• Cosmological mass limits on neutrinos, axions, and other light particles
• CMB Signals of Neutrino Mass Generation
• Distinguishing different scenarios of early energy release with spectral distortions of the cosmic microwave background
• Phantom k-essence cosmologies
• FRW Bulk Viscous Cosmology with Modified Chaplygin Gas in Flat Space
• An Inflationary Model in String Theory
• Dynamics of Bianchi I Universe with Magnetized Anisotropic Dark Energy
• Constraints on cosmic hemispherical power anomalies from quasars
• Interacting tachyon dark energy in non-flat universe
• WIMP diffusion in the solar system including solar depletion and its effect on Earth capture rates
• Searching for Dark Matter with Future Cosmic Positron Experiments
• Exact solutions of f(R) gravity coupled to nonlinear electrodynamics
• Reionisation, chemical enrichment and seed black holes from the first stars: is Population III important?
• The Holographic dark energy reexamined
• Anisotropic cosmological models in $f(R,T)$ gravity with variable deceleration parameter
• The Keck+Magellan Survey for Lyman Limit Absorption I: The Frequency Distribution of Super Lyman Limit Systems
• Full one-loop corrections to the relic density in the MSSM: A few examples
• Low-order multipole maps of CMB anisotropy derived from WMAP
• Lower limits on the Hubble Constant from models of Type Ia Supernovae
• Loop Quantum Cosmology, Boundary Proposals, and Inflation
• Kerr-de Sitter Universe
• Quintessential inflation with canonical and noncanonical scalar fields and Planck 2015 results
• The Statistical Significance of the Low CMB Mulitipoles
• Holographic dark energy in Brans-Dicke cosmology with chameleon scalar field
• Can a matter-dominated model with constant bulk viscosity drive the accelerated expansion of the universe?
• Primordial Neutrinos
• Hybrid modified gravity unifying local tests, galactic dynamics and late-time cosmic acceleration
• On holographic dark-energy models
• Scaling Laws in the Distribution of Galaxies
• Some exact solutions of F(R) gravity with charged (a)dS black hole interpretation
• Exploring Cluster Physics with High-Resolution Sunyaev-Zel'dovich Effect Images and X-Ray Data: The Case of the Most X-Ray-Luminous Galaxy Cluster RX J1347-1145
• WMAPping inflationary physics
• Searches for the role of spin and polarization in gravity
• Dark Matter Subhaloes in Numerical Simulations
• Probing the curvature and dark energy
• Bayesian analysis of an anisotropic universe model: systematics and polarization
• Relic gravitational waves and their detection
• A preference for a non-zero neutrino mass from cosmological data
• The Beginning and Evolution of the Universe
• Dark Matter in the Finely Tuned Minimal Supersymmetric Standard Model
• Bouncing cosmology in $f(R,T)$ gravity
• Seeking String Theory in the Cosmos
• Phenomenology of TeV Right-handed Neutrino and the Dark Matter Model
• Direct Detection of Dark Matter in Supersymmetric Models
• Interacting dark energy in $f(R)$ gravity
• Phantom Field with O(N) Symmetry in Exponential Potential
• First Detection of Polarization of the Submillimetre Diffuse Galactic Dust Emission by Archeops
• Non-Gaussian Error Distribution of Hubble Constant Measurements
• Intracluster and Intragroup Entropy from Quasar Activity
• The Richness-Dependent Cluster Correlation Function: Early SDSS Data
• Thermodynamical Interpretation of the Interacting Holographic Dark Energy Model in a non-flat Universe
• Spacetime foam: from entropy and holography to infinite statistics and nonlocality
• Holographic Foam, Dark Energy and Infinite Statistics
• Noether symmetry in $f(R)$ cosmology
• Exploring a matter-dominated model with bulk viscosity to drive the accelerated expansion of the Universe
• Brane Inflation and Cosmic String Tension in Superstring Theory
• High-Energy Cosmic Rays from Gamma-Ray Bursts
• Second Order General Slow-Roll Power Spectrum
• Diurnal and Annual Modulation of Cold Dark Matter Signals
• Constraints on the sound speed of dark energy
• Green's function of the cosmological thermalization problem
• Indirect Sensitivities to the Scale of Supersymmetry
• Modified Chaplygin Gas Cosmology
• Proper Motions of Dwarf Spheroidal Galaxies from Hubble Space Telescope Imaging. III: Measurement for Ursa Minor
• The Supersymmetric Parameter Space in Light of B-physics Observables and Electroweak Precision Data
• Stability of a non-minimally conformally coupled scalar field in F(T) cosmology
• Self sustained phantom wormholes in semi-classical gravity
• Bounds on isocurvature perturbations from CMB and LSS data
• Dark Energy Tomography
• Unification of inflation and cosmic acceleration in the Palatini formalism
• Phantom stars and topology change
• Detection of the ISW effect and corresponding dark energy constraints made with directional spherical wavelets
• Detection of the ISW effect and corresponding dark energy constraints
• Two-Fluid Scenario for Dark Energy Models in an FRW Universe-Revisited
• The CMB cold spot: texture, cluster or void?
• Cosmic Microwave Background, Accelerating Universe and Inhomogeneous Cosmology
• Observational constraints on the acceleration of the Universe
• Finite-time Cosmological Singularities and the Possible Fate of the Universe
• Direct Detection of the Wino- and Higgsino-like Neutralino Dark Matters at One-Loop Level
• Noether symmetry of F(T) cosmology with quintessence and phantom scalar fields
• Which cosmological model with dark energy -- phantom or LambdaCDM
• Cosmological parameter estimation using Very Small Array data out to l=1500
• Mass-to-light ratio gradients in early-type galaxy haloes
• Lines in the cosmic microwave background spectrum from the epoch of cosmological helium recombination
• Mitigating Foreground Biases in CMB Lensing Reconstruction Using Cleaned Gradients
• Generalized Slow Roll for Large Power Spectrum Features
• New holographic scalar field models of dark energy in non-flat universe
• Exploring the BWCA (Bino-Wino Co-Annihilation) Scenario for Neutralino Dark Matter
• Cosmology of the Very Early Universe
• Carbon monoxide line emission as a CMB foreground: tomography of the star-forming universe with different spectral resolutions
• A Near-Infrared Analysis of the Submillimeter Background and the Cosmic Star-Formation History
• Comparison of SUSY spectrum calculations and impact on the relic density constraints from WMAP
• Modified gravity and the stability of de Sitter space
• Interacting Ghost Dark Energy in Non-Flat Universe
• Escaping the Big Rip?
• Reconstructing the primordial power spectrum - a new algorithm
• Detectability of Long GRB Afterglows from Very High Redshifts
• Slow-roll parameters in braneworld cosmologies
• Thermodynamical properties of the Universe with dark energy
• Solar Neutrino Constraints on the BBN Production of Li
• Neutrino Dark Energy -- Revisiting the Stability Issue
• Stringy Effects During Inflation and Reheating
• Signals From the Epoch of Cosmological Recombination
• Gauss-Bonnet Gravitational Baryogenesis
• Fourier analysis of luminosity-dependent galaxy clustering
• Possible Explanation to Low CMB Quadrupole
• Likelihood Analysis of the CMSSM Parameter Space
• Future Type Ia Supernova Data as Tests of Dark Energy from Modified Friedmann Equations
• Bayesian model selection and isocurvature perturbations
• Detecting Population III stars through observations of near-IR cosmic infrared background anisotropies
• Anisotropic Universe Models with Perfect Fluid and Scalar Field in f(R,T) Gravity
• Massive Particle Decay and Cold Dark Matter Abundance
• The Matter Bounce Alternative to Inflationary Cosmology
• A comprehensive set of elemental abundances in damped Ly-alpha systems: revealing the nature of these high-redshift galaxies
• Bianchi Type-I Anisotropic Dark Energy Models with Constant Deceleration Parameter
• Inflationary spectra and violations of Bell inequalities
• Assessing the effects of foregrounds and sky removal in WMAP
• Interacting agegraphic tachyon model of dark energy
• Thermal history of the plasma and high-frequency gravitons
• Unification of inflation and dark energy {\it à la} quintessential inflation
• Inhomogeneity effects in Cosmology
• Constraints on mode couplings and modulation of the CMB with WMAP data
• Multipole vector anomalies in the first-year WMAP data: a cut-sky analysis
• Exploring the Superimposed Oscillations Parameter Space
• A comparison of cosmological Boltzmann codes: are we ready for high precision cosmology?
• Gravitational waves and stalled satellites from massive galaxy mergers at z <= 1
• Non-minimally Coupled Quintom Model Inspired by String Theory
• Theoretical predictions for the direct detection of neutralino dark matter in the NMSSM
• Correlated Primordial Perturbations in Light of CMB and LSS Data
• Reasoning From Fossils: Learning From the Local Black Hole Population About the Evolution of Quasars
• Future Evolution of Structure in an Accelerating Universe
• Shock-Heated Gas in the Large Scale Structure of the Universe
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: On-Orbit Radiometer Characterization
• Higgsino Dark Matter in a SUGRA Model with Nonuniversal Gaugino Masses
• The Caustic Ring Model of the Milky Way Halo
• The Holographic Model of Dark Energy and Thermodynamics of Non-Flat Accelerated Expanding Universe
• Searching for a holographic connection between dark energy and the low-l CMB multipoles
• Invisible Quarkonium Decays as a Sensitive Probe of Dark Matter
• Recovering the Inflationary Potential and Primordial Power Spectrum With a Slow Roll Prior: Methodology and Application to WMAP 3 Year Data
• The N-point correlation functions of the first-year Wilkinson Microwave Anisotropy Probe sky maps
• Representations of spectral coordinates in FITS
• Statistical Isotropy of the Wilkinson Microwave Anisotropy Probe Data: A Bipolar Power Spectrum Analysis
• The 7Be(d,p)2alpha cross section at Big Bang energies and the primordial 7Li abundance
• Structure formation constraints on the Jordan-Brans-Dicke theory
• A Note on Crossing the Phantom Divide in Hybrid Dark Energy Model
• New agegraphic dark energy in Horava-Lifshitz cosmology
• Comparison of Approaches to Quantum Correction of Black Hole Thermodynamics
• Probing the Local Group Medium Toward Mkn 421 with Chandra and FUSE
• First measurements of the polarization of the cosmic microwave background radiation at small angular scales from CAPMAP
• Black holes in the presence of dark energy
• Centimeter-wave continuum radiation from the rho Ophiuchi molecular cloud
• The Constancy of the Constants of Nature: Updates
• Radio Observations of the 13hr XMM/ROSAT Deep X-ray Survey Area
• Newtonian limit of the singular f(R) gravity in the Palatini formalism
• Cosmology from Rolling Massive Scalar Field on the anti-D3 Brane of de Sitter Vacua
• Supernovae constraints on models of dark energy revisited
• Testing the dark energy with gravitational lensing statistics
• Measuring $\alpha$ in the Early Universe: CMB Polarization, Reionization and the Fisher Matrix Analysis
• Modified equation of state, scalar field, and bulk viscosity in Friedmann universe
• Reconstructing Sparticle Mass Spectra using Hadronic Decays
• Measuring dark energy properties with 3D cosmic shear
• Stability properties of some perfect fluid cosmological models
• Reconstruction of Hessence Dark Energy and the Latest Type Ia Supernovae Gold Dataset
• Neutrino Masses and Mixings in a Predictive SO(10) Model with CKM CP Violation
• Prediction of the Cosmic Evolution of the CO-Luminosity Functions
• $f(T)$ gravitational baryogenesis
• D-term inflation without cosmic strings
• K-Chameleon and the Coincidence Problem
• Exact likelihood evaluations and foreground marginalization in low resolution WMAP data
• Viscous FRW Cosmology in Modified Gravity
• Holographic principle and dark energy
• A Modified Holographic Dark Energy Model with Infrared Infinite Extra Dimension(s)
• Testing Primordial Non-Gaussianity in CMB Anisotropies
• Probing spacetime foam with extragalactic sources
• Baryon oscillations
• 5-dimensional Brans-Dicke Theory and Cosmic Acceleration
• Sub-millimeter to centimeter excess emission from the Magellanic Clouds. I. Global spectral energy distribution
• Cross-correlation of CMB with large-scale structure: weak gravitational lensing
• Interacting model of new agegraphic dark energy: Cosmological evolution and statefinder diagnostic
• Early star formation traced by the highest redshift quasars
• Velocity Dispersion of 335 Galaxy Clusters Selected from the Sloan Digital Sky Survey: Statistical Evidence for Dynamical Interaction, and Against Ram-Pressure Stripping
• Indication for Primordial Anisotropies in the Neutrino Background from WMAP and SDSS
• Noether Symmetry Approach in $f(\mathcal{G},T)$ Gravity
• Evolution in the Color-Magnitude Relation of Early-Type Galaxies in Clusters of Galaxies at z~=1
• The deuterium-to-oxygen ratio in the interstellar medium
• Decaying particles and the reionization history of the Universe
• Hunting for the Top Partner in the Littlest Higgs Model with T-parity at the LHC
• Effective Action and Soft Supersymmetry Breaking for Intersecting D-brane Models
• Fast cosmological parameter estimation using neural networks
• Singularity free anisotropic strange quintessence star
• Constraints on a mixed inflaton and curvaton scenario for the generation of the curvature perturbation
• Testable polarization predictions for models of CMB isotropy anomalies
• The effects of spatial resolution on Integral Field Spectrograph surveys at different redshifts. The CALIFA perspective
• CP-odd Phase Correlations and Electric Dipole Moments
• Phenomenology of amplitude-corrected post-Newtonian gravitational waveforms for compact binary inspiral. I. Signal-to-noise ratios
• Extending the WMAP Bound on the Size of the Universe
• WMAP Constraints on varying $\alpha$ and the Promise of Reionization
• Higher order corrections of the extended Chaplygin gas cosmology with varying $G$ and $\Lambda$
• Phantom field dynamics in loop quantum cosmology
• On the generalised Chaplygin gas: worse than a big rip or quieter than a sudden singularity?
• Realistic cosmological scenario with non-minimal kinetic coupling
• Missing Thermal Energy of the Intracluster Medium
• Relic abundance of dark matter in the minimal universal extra dimension model
• Missing Baryons and the Warm-Hot Intergalactic Medium
• Evolution of Second-Order Cosmological Perturbations and Non-Gaussianity
• Apparent cosmic acceleration from type Ia supernovae
• CMBR Constraint on a Modified Chaplygin Gas Model
• An analysis of the evolving comoving number density of galaxies in hydrodynamical simulations
• Structure formation in a string-inspired modification of the cold dark matter model
• Constraints on the coupled quintessence from cosmic microwave background anisotropy and matter power spectrum
• Very Large Primordial Non-Gaussianity from multi-field: Application to Massless Preheating
• A high-significance detection of non-Gaussianity in the WMAP 5-year data using directional spherical wavelets
• Constraints on the Variation of G from Primordial Nucleosynthesis
• Non-Vacuum Bianchi Types I and V in f(R) Gravity
• Ginzburg-Landau Theory of Dark Energy: A Framework to Study Both Temporal and Spatial Cosmological Tensions Simultaneously
• Fast and Efficient Template Fitting of Deterministic Anisotropic Cosmological Models Applied to WMAP Data
• Neutralino Annihilation at the Galactic Center Revisited
• Analytic approach to the CMB polarizations generated by relic gravitational waves
• The Fall of Stringy de Sitter
• Slow Roll Reconstruction: Constraints on Inflation from the 3 Year WMAP Dataset
• WMAP constraints on scalar-tensor cosmology and the variation of the gravitational constant
• Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
• Upper Bound On Gluino Mass From Thermal Leptogenesis
• The Parsec-Scale Jets of the TeV Blazars H 1426+428, 1ES 1959+650, and PKS 2155-304: 2001-2004
• Non-Gaussianity from Cosmic Magnetic Fields
• Can Gamma-Ray Bursts Be Used to Measure Cosmology? A Further Analysis
• A re-analysis of the three-year WMAP temperature power spectrum and likelihood
• Bianchi Type I Cosmology in Generalized Saez-Ballester Theory via Noether Gauge Symmetry
• Implications of a Running Spectral Index for Slow Roll Inflation
• The UCSD Radio-Selected Quasar Survey for Damped Lyman alpha System
• The Peccei-Quinn Field as Curvaton
• The power spectrum and bispectrum of SDSS DR11 BOSS galaxies II: cosmological interpretation
• Improved Measurement of the Spectral Index of the Diffuse Radio Background Between 90 and 190 MHz
• Some Exact Solutions in $f(\mathcal{G},T)$ Gravity via Noether Symmetries
• Can superhorizon perturbations drive the acceleration of the Universe?
• The Full Second-Order Radiation Transfer Function for Large-Scale CMB Anisotropies
• Decoupling in an expanding universe: boundary RG-flow affects initial conditions for inflation
• Constraints on Supersymmetric Grand Unified Theories from Cosmology
• CKM CP Violation in a Minimal SO(10) Model for Neutrinos and Its Implications
• Broken Isotropy from a Linear Modulation of the Primordial Perturbations
• Supersymmetric Benchmarks with Non-Universal Scalar Masses or Gravitino Dark Matter
• The Atacama Cosmology Telescope Project: A Progress Report
• Light element evolution resulting from WMAP data
• Estimation of Primordial Spectrum with post-WMAP 3 year data
• Non-Gaussian perturbations in hybrid inflation
• Observational constraints on patch inflation in noncommutative spacetime
• Theoretical Limits on the Equation-of-State Parameter of Phantom Cosmology
• Primordial fluctuations and cosmological inflation after WMAP 1.0
• The State Equation of the Yang-Mills field Dark Energy Models
• SZ and CMB reconstruction using Generalized Morphological Component Analysis
• $f(R)$ gravity constrained by PPN parameters and stochastic background of gravitational waves
• Bayesian Power Spectrum Analysis of the First-Year WMAP data
• Relaxing Constraints on Inflation Models with Curvaton
• Relativistic second-order perturbations of nonzero-Λflat cosmological models and CMB anisotropies
• Polar Dust, Nuclear Obscuration and IR SED Diversity in Type-1 AGNs
• Cosmological Evolution of Interacting New Holographic Dark Energy in Non-flat Universe
• A 5% measurement of the Hubble constant from Type II supernovae
• A new measurement of the expansion history of the Universe at z=1.26 with cosmic chronometers in VANDELS
• Accretion and Evaporation of Modified Hayward Black Hole
• Tracking quintessence by cosmic shear - Constraints from VIRMOS-Descart and CFHTLS and future prospects
• CMB Constraints on the Holographic Dark Energy Model
• The Near Infrared Background: Interplanetary Dust or Primordial Stars?
• Magnetized CMB observables: a dedicated numerical approach
• Requirements on collider data to match the precision of WMAP on supersymmetric dark matter
• The age of the Milky Way halo stars from the Sloan Digital Sky Survey
• Inflation from R^2 gravity: a new approach using nonlinear electrodynamics
• On the Viability of Bianchi Type VIIh Models with Dark Energy
• Split Two-Higgs-Doublet Model and Neutrino Condensation
• f(R) Gravity: From the Pioneer Anomaly to the Cosmic Acceleration
• FRW Quantum Cosmology with a Generalized Chaplygin Gas
• Holographic dark energy with varying gravitational constant in Horava-Lifshitz cosmology
• Particle decay in inflationary cosmology
• Cosmological perturbations from varying masses and couplings
• Stabilizing the invisible axion in 3-3-1 models
• Primordial magnetic field and non-Gaussianity of the 1-year Wilkinson Microwave Anisotropy Probe (WMAP) data
• Dynamics of interacting phantom scalar field dark energy in Loop Quantum Cosmology
• All in action
• Primordial black hole constraints with Hawking radiation -- a review
• Morphologies and Color Gradients of Luminous Evolved Galaxies at z~1.5
• Mapping the large-scale anisotropy in the WMAP data
• Inflaton field potential producing the exactly flat spectrum of adiabatic perturbations
• New agegraphic dark energy model with generalized uncertainty principle
• Scalar Tensor Teleparallel Dark Gravity via Noether Symmetry
• A Possible Explanation of Low Energy $\gamma$-ray Excess from Galactic Centre and Fermi Bubble by a Dark Matter Model with Two Real Scalars
• Phenomenological viability of neutralino dark matter in the NMSSM
• Brans-Dicke Theory as a Unified Model for Dark Matter - Dark Energy
• Phenomenological Constraints on Patterns of Supersymmetry Breaking
• On the generation of density perturbations at the end of inflation
• Analyze This! A Cosmological Constraint Package for CMBEASY
• Cosmology of Holographic and New Agegraphic $f(R,T)$ Models
• Energy conditions in f(R) gravity and Brans-Dicke theories
• Cosmological Evolution in f(R,T) theory with Collisional Matter
• Self-annihilation of the neutralino dark matter into two photons or a Z and a photon in the MSSM
• Significant effects of second KK particles on LKP dark matter physics
• Hubble flow variance and the cosmic rest frame
• Topology and Geometry of Gaussian random fields I: on Betti Numbers, Euler characteristic and Minkowski functionals
• Fast directional continuous spherical wavelet transform algorithms
• Fast optimal CMB power spectrum estimation with Hamiltonian sampling
• Initial state of matter fields and trans-Planckian physics: Can CMB observations disentangle the two?
• M/String Theory, S-branes and Accelerating Universe
• A 2500 square-degree CMB lensing map from combined South Pole Telescope and Planck data
• Unbiased Estimation of an Angular Power Spectrum
• Measurement of the $T_{\mathrm{CMB}}$ evolution from the Sunyaev-Zel'dovich effect
• CMB Anisotropy of the Poincare Dodecahedron
• D-branes in Standard Model building, Gravity and Cosmology
• Accelerating Universe in Modified Theories of Gravity
• The Lyth Bound Revisited
• Revisit of the interacting holographic dark energy model after Planck 2015
• Gravitational waves from dark matter isocurvature
• Constraints on isocurvature models from the WMAP first-year data
• Constraints on the Primordial Power Spectrum from High Resolution Lyman-alpha Forest Spectra and WMAP
• On Special Relativity with Cosmological Constant
• Very Constrained Minimal Supersymmetric Standard Models
• Non-linear inflationary perturbations
• On the CMB large-scales angular correlations
• Constraints on non-flat cosmologies with massive neutrinos after Planck 2015
• Cardy-Verlinde Formula and Holographic Dark Energy
• The ISOPHOT-MAMBO survey of 3CR radio sources: Further evidence for the unified schemes
• Inflationary universe in loop quantum cosmology
• Hybrid Estimation of CMB Polarization Power Spectra
• Gravitational lensing in fourth order gravity
• Long life stau in the minimal supersymmetric standard model
• Conserved Quantities in $f(R)$ Gravity via Noether Symmetry
• Cosmic Positron Signature from Dark Matter in the Littlest Higgs Model with T-parity
• Constraining dark energy with Hubble parameter measurements: an analysis including future redshift-drift observations
• On the Stability of Phantom K-essence Theories
• Probing Dark Energy Using Its Density Instead of Its Equation of State
• Results from the Wilkinson Microwave Anisotropy Probe
• The Interstellar Magnetic Field Close to the Sun II
• A 2% Distance to z = 0.35 by Reconstructing Baryon Acoustic Oscillations - III : Cosmological Measurements and Interpretation
• Kaluza-Klein cosmological model in $f(R,T)$ gravity with $\Lambda (T)$
• Supersymmetric Dark Matter and the Extragalactic Gamma Ray Background
• Bulk viscous matter and recent acceleration of the Universe
• An Interacting Two-Fluid Scenario for Dark Energy in FRW Universe
• The Beginning and the End: The Meaning of Life in a Cosmological Perspective
• Mixed Wino Dark Matter: Consequences for Direct, Indirect and Collider Detection
• Superposition of blackbodies and the dipole anisotropy: A possibility to calibrate CMB experiments
• Precession in the inner jet of 3C 345
• Lepton Flavor Violating Processes and Muon g-2 in Minimal Supersymmetric SO(10) Model
• Interacting new agegraphic dark energy in non-flat Brans-Dicke cosmology
• CPT Violation and Decoherence in Quantum Gravity
• MCMC analysis of WMAP3 and SDSS data points to broken symmetry inflaton potentials and provides a lower bound on the tensor to scalar ratio
• Disks in the sky: A reassessment of the WMAP "cold spot"
• The X-ray view of Giga-Hertz Peaked Spectrum Radio Galaxies
• Alignment tests for low CMB multipoles
• Sub-parsec radio cores in nearby Seyfert galaxies
• Neutrino mass limits from SDSS, 2dFGRS and WMAP
• Can Supersymmetry Naturally Explain the Positron Excess?
• Supersymmetric Thermalization and Quasi-Thermal Universe: Consequences for Gravitinos and Leptogenesis
• Dark Energy Model in Anisotropic Bianchi Type-III Space-Time with Variable EoS Parameter
• Implications of the Curvaton on Inflationary Cosmology
• Dark Energy: Recent Developments
• Interacting Ghost Dark Energy in Brans-Dicke Theory
• Accelerated Cosmological Models in Modified Gravity tested by distant Supernovae SNIa data
• ROMA: a map-making algorithm for polarised CMB data sets
• The search for habitable worlds: 1. The viability of a starshade mission
• A needlet ILC analysis of WMAP 9-year polarisation data: CMB polarisation power spectra
• Systematics of Constant Roll Inflation
• Dark Matter in B-L Extended MSSM Models
• A high-significance detection of non-Gaussianity in the WMAP 3-year data using directional spherical wavelets
• Bounds on CDM and neutrino isocurvature perturbations from CMB and LSS data
• Cosmological Evolution of Interacting Dark Energy Models with Mass Varying Neutrinos
• Power spectrum of the maxBCG sample: detection of acoustic oscillations using galaxy clusters
• Quintom dark energy models with nearly flat potentials
• Non-minimal quintessence and phantom with nearly flat potentials
• Quintessence Models and the Cosmological Evolution of alpha
• Curvature driven acceleration : a utopia or a reality ?
• Gauge-invariant Formulation of the Second-order Cosmological Perturbations
• Constraints on the Evolution of the Primordial Magnetic Field from the Small-Scale Cosmic Microwave Background Angular Anisotropy
• Faraday rotation, stochastic magnetic fields and CMB maps
• Split Supersymmetry, stable gluino, and gluinonium
• Making sky maps from Planck data
• Relic density of dark matter in brane world cosmology
• Testing loop quantum cosmology
• The Birmingham-CfA cluster scaling project - II. Mass composition and distribution
• Stochastic backgrounds of relic gravitons: a theoretical appraisal
• Constraining evolution in the Halo Model using galaxy redshift surveys
• Squeezing the window on isocurvature modes with the Lyman-alpha forest
• Warping and precession in galactic and extragalactic accretion disks
• Explaining Cosmological Anisotropy: Evidence for Causal Horizons from CMB data
• CMB quadrupole suppression: I. Initial conditions of inflationary perturbations
• The matter distribution in the local Universe as derived from galaxy groups in SDSS DR12 and 2MRS
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• The soft X-ray excess: NLS1s vs. BLS1s
• Same-sign top quarks as signature of light stops at the CERN LHC
• Reappraising foreground contamination in the COBE-DMR data
• Constraints on the DGP Model from Recent Supernova Observations and Baryon Acoustic Oscillations
• A low CMB variance in the WMAP data
• Features in Dark Energy Equation of State and Modulations in the Hubble Diagram
• Density Perturbations for Running Cosmological Constant
• Characterizing Inflationary Perturbations: The Uniform Approximation
• The bouncing cosmology with $F(R)$ gravity and its reconstructing
• Narrow Line Seyfert 1 galaxies at hard X-rays
• Shadow of a Charged Rotating Black Hole in $f(R)$ Gravity
• CMB Anisotropy of Spherical Spaces
• Primordial backgrounds of relic gravitons
• Reconstructing the Primordial Spectrum from WMAP Data by the Cosmic Inversion Method
• Galaxy clustering constraints on deviations from Newtonian gravity at cosmological scales
• The Relevance of the Cosmological Constant for Lensing
• The hard X-ray view of Giga-Hertz Peaked Spectrum Radio Galaxies
• Interacting new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe
• Dark Energy Stars in Tolman-Kuchowicz spacetime in the context of Einstein Gravity
• CMB Observations and the Production of Chemical Elements at the End of the Dark Ages
• Thermal leptogenesis in a model with mass varying neutrinos
• Cosmological Parameter Constraints as Derived from the Wilkinson Microwave Anisotropy Probe Data via Gibbs Sampling and the Blackwell-Rao Estimator
• Towards inflation and dark energy cosmologies from modified Gauss-Bonnet theory
• Gravitino Dark Matter Scenarios with Massive Metastable Charged Sparticles at the LHC
• Gravitational energy as dark energy: Concordance of cosmological tests
• Notes on dark energy interacting with dark matter and unparticle in loop quantum cosmology
• CMB quadrupole suppression: II. The early fast roll stage
• Non-parametric reconstruction of the primordial power spectrum at horizon scales from WMAP data
• A New Independent Limit on the Cosmological Constant/Dark Energy from the Relativistic Bending of Light by Galaxies and Clusters of Galaxies
• Dynamical Relaxation of Dark Energy: A Solution to Early Inflation, Late-time Acceleration and the Cosmological Constant Problem
• Time-delay cosmographic forecasts with strong lensing and JWST stellar kinematics
• CMB power spectrum estimation using wavelets
• Chaotic hybrid new inflation in supergravity with a running spectral index
• Interacting entropy-corrected agegraphic-tachyon dark energy
• Large Angle CMB Fluctuations from Cosmic Strings with a Comological Constant
• Accelerating dark energy models in bianchi Type-V space-time
• On the significance of power asymmetries in Planck CMB data at all scales
• CMB-slow, or How to Estimate Cosmological Parameters by Hand
• Post-WMAP Assessment of Infrared Cutoff in the Primordial Spectrum from Inflation
• Cosmic Acceleration from M Theory on Twisted Spaces
• Alleviation of Cosmic Age Problem In Interacting Dark Energy Model
• CMB Maximum Temperature Asymmetry Axis: Alignment with Other Cosmic Asymmetries
• A panchromatic view of PKS 0558-504: an ideal laboratory to study the disk-jet link
• Broadband study of hard X-ray selected absorbed AGN
• A Deep Search for Extended Radio Continuum Emission From Dwarf Spheroidal Galaxies: Implications for Particle Dark Matter
• Inflation from Superstring/M-Theory Compactification with Higher Order Corrections II -- Case of Quartic Weyl Terms --
• Natural Multi-Higgs Model with Dark Matter and CP Violation
• ISW measurements with photometric redshift surveys: 2MASS results and future prospects
• On Precision Measurement of the Mean Curvature
• Accelerating universe from gravitational leakage into extra dimensions: confrontation with SNeIa
• Observational constraints on the interacting Ricci dark energy model
• Analytical solutions of the geodesic equation in the spacetime of a black hole in f(R) gravity
• How clustering dark energy affects matter perturbations
• Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
• Cosmo-dynamics and dark energy with a quadratic EoS: anisotropic models, large-scale perturbations and cosmological singularities
• Towards a Precision Cosmology from Starburst Galaxies at z>2
• Measuring the primordial power spectrum: Principal component analysis of the cosmic microwave background
• Accretion of New Variable Modified Chaplygin Gas and Generalized Cosmic Chaplygin Gas onto Schwarzschild and Kerr-Newman Black holes
• A Quintom scenario with mixed kinetic terms
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Signal Contamination from Sidelobe Pickup
• Limiting the dimming of distant type Ia supernovae
• Star Models with Dark Energy
• Constraints on Scalar-Field Dark Energy from Galaxy Cluster Gas Mass Fraction versus Redshift
• Unparticle Dark Matter
• ChaMP Serendipitous Galaxy Cluster Survey
• Accelerating Universes and String Theory
• Models of Baryogenesis via Spontaneous Lorentz Violation
• Flipped SU(5) Predicts $\delta T/T$
• Anisotropic perturbations due to dark energy
• Optical Properties of 4248 IRAS Galaxies
• Aspects of Cosmic Inflation in Expanding Bose-Einstein Condensates
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids
• Barrow HDE model for Statefinder diagnostic in FLRW Universe
• The generalized second law of gravitational thermodynamics on the apparent and event horizons in FRW cosmology
• Effects of a pre-inflation radiation-dominated epoch to CMB anisotropy
• On Star Formation and the Non-Existence of Dark Galaxies
• Detection and discrimination of cosmological non-Gaussian signatures by multi-scale methods
• Gravitational Baryogenesis in Non-Minimal Coupled $f(R,T)$ Gravity
• A New Approach to Quintessence and a Solution of Multiple Attractors
• Gravitational waves, inflation and the cosmic microwave background: towards testing the slow-roll paradigm
• Correspondence between entropy-corrected holographic and Gauss-Bonnet dark energy models
• Measuring our peculiar velocity on the CMB with high-multipole off-diagonal correlations
• Phase cross-correlation of the WMAP ILC map and foregrounds
• Modified gravity with $f(R)=\sqrt{R^2-R_0^2}$
• Far-Ultraviolet & X-ray Observations of VV 114: Feedback in a Local Analog to Lyman Break Galaxies
• $f(R,T)$ models applied to Baryogenesis
• Holographic hessence models
• How can gravitational-wave standard sirens and 21 cm intensity mapping jointly provide a precise late-universe cosmological probe?
• Large-Angle Correlations in the Cosmic Microwave Background
• Beryllium in turnoff stars of NGC6397: early Galaxy spallation, cosmochronology and cluster formation
• Crossing of the w=-1 barrier in viscous modified gravity
• Cosmography approach to dark energy cosmologies: new constrains using the Hubble diagrams of supernovae, quasars and gamma-ray bursts
• The CMB temperature power spectrum from an improved analysis of the Archeops data
• Empirical Foundations of Relativistic Gravity
• Dynamics of Quintom and Hessence Energies in Loop Quantum Cosmology
• Anomaly of Zbb coupling revisited in MSSM and NMSSM
• The Sunyaev-Zel'dovich effect in a sample of 31 clusters - a comparison between the X-ray predicted and WMAP observed CMB temperature decrement
• Black Hole Formation from Collapsing Dust Fluid in a Background of Dark Energy
• On compatibility of string effective action with an accelerating universe
• Foreground Subtraction of Cosmic Microwave Background Maps using WI-FIT (Wavelet based hIgh resolution Fitting of Internal Templates)
• Remarks on the formulation of the cosmological constant/dark energy problems
• Probing the curvature of the Universe from supernova measurement
• Cosmological Backreaction from Perturbations
• Inflation model with lower multipoles of the CMB suppressed
• Direct and Indirect Detection of Neutralino Dark Matter In Selected Supersymmetry Breaking Scenarios
• The Cosmic Reionization History as Revealed by the CMB Doppler--21-cm Correlation
• Future CMB constraints on cosmic birefringence and implications for fundamental physics
• LRS Bianchi type I universes exhibiting Noether symmetry in the scalar-tensor Brans-Dicke theory
• Cosmological perturbations from stochastic gravity
• Casimir energy-momentum tensor for a brane in de Sitter spacetime
• uvby-βphotometry of high-velocity and metal-poor stars XI. Ages of halo and old disk stars
• Shift Symmetry and Inflation in Supergravity
• The eccentric universe
• Isotropy of the early universe from CMB anisotropies
• Nucleosynthesis Without a Computer
• Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars
• Could dark energy be measured in the lab?
• Attractor solutions for general hessence dark energy
• XMM-Newton broad-band observations of NGC 7582: Nh variations and fading out of the active nucleus
• Thermalization of large energy release in the early Universe
• Hints of Isocurvature Perturbations in the Cosmic Microwave Background?
• Dark Energy Constraints from Baryon Acoustic Oscillations
• Median Statistics and the Mass Density of the Universe
• Current Observational Constraints on Cosmic Doomsday
• Large-scale inhomogeneities in modified Chaplygin gas cosmologies
• Relic Abundance of LKP Dark Matter in UED model including Effects of Second KK Resonances
• Realistic Yukawa Textures and SUSY Spectra from Intersecting Branes
• Measurement of the electron-pressure profile of galaxy clusters in Wilkinson Microwave Anisotropy Probe (WMAP) 3-year data
• Physics Impact of a Precise Determination of the Top Quark Mass at an e+e- Linear Collider
• Gamma-ray Astrophysics in the MeV Range: the ASTROGAM Concept and Beyond
• Spectroscopy of luminous z>7 galaxy candidates and sources of contamination in z>7 galaxy searches
• A Detection of the Integrated Sachs-Wolfe Effect
• An alternative to the LCDM model: the case of scale invariance
• Forecasting performance of CMB experiments in the presence of complex foreground contaminations
• Alpha-states in de Sitter space
• The Multipole Vectors of WMAP, and their frames and invariants
• Deep Chandra and multicolor HST follow-up of the jets in two powerful radio quasars
• Cheng-Weyl Vector Field and its Cosmological Application
• Supersymmetry Simulations with Off-Shell Effects for LHC and ILC
• Template fitting and the large-angle CMB anomalies
• WMAP Dark Matter Constraints and Yukawa Unification in SUGRA models with CP Phases
• Stability Analysis in Tachyonic Potential Chameleon cosmology
• Modelling of the Spectral Energy Distribution of Fornax A: Leptonic and Hadronic Production of High Energy Emission from the Radio Lobes
• Supernova Ia and Galaxy Cluster Gas Mass Fraction Constraints on Dark Energy
• Measuring Dark Energy with Gamma-Ray Bursts and Other Cosmological Probes
• Consistency of $f(R)=\sqrt{R^2-R_0^2}$ Gravity with the Cosmological Observations in Palatini Formalism
• Exact scaling solutions and fixed points for general scalar field
• Alignment and signed-intensity anomalies in WMAP data
• Looking for Cosmological Alfven Waves in WMAP Data
• Parity Asymmetry in the CMBR Temperature Power Spectrum
• Constraints on the Topology of the Universe: Extension to General Geometries
• More on the initial singularity problem in gravity's rainbow cosmology
• Dissipative or Conservative cosmology with dark energy ?
• Unified dark fluid in Brans-Dicke theory
• Detecting the Cosmic Dipole Anisotropy in Large-Scale Radio Surveys
• Asymmetric inflation: exact solutions
• Inflationary Potential Reconstruction for a WMAP Running Power Spectrum
• Cosmology with nonminimal kinetic coupling and a power-law potential
• Cleaned Three-Year WMAP CMB Map: Magnitude of the Quadrupole and Alignment of Large Scale Modes
• High-resolution asymptotics for the angular bispectrum of spherical random fields
• The radio relic in Abell 2256: overall spectrum and implications for electron acceleration
• Cosmological evolution and statefinder diagnostic for new holographic dark energy model in non flat universe
• Confrontation of MOND Predictions with WMAP First Year Data
• The Inner Caustics of Cold Dark Matter Halos
• A blind estimation of the power spectrum of CMB anisotropy from WMAP
• Cosmological constraints combining H(z), CMB shift and SNIa observational data
• The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens
• Acceleration of the universe in the Einstein frame of a metric-affine f(R) gravity
• Testing power-law cosmology with galaxy clusters
• Anomalies in the low CMB multipoles and extended foregrounds
• Generalized Chaplygin gas model, supernovae and cosmic topology
• Yang-Mills condensate dark energy coupled with matter and radiation
• Large scale anomalies in the CMB and non-Gaussianity in bouncing cosmologies
• Polynomial Interpretation of Multipole Vectors
• Constraints on Cardassian Scenario from the Expansion Turnaround Redshift and the Sunyaev-Zeldovich/X-ray Data
• Well-proportioned universes suppress CMB quadrupole
• Low Frequency Radio Observations of X-ray Ghost Bubbles in Abell 2597: A History of Radio Activity in the Core
• Dark Energy or Apparent Acceleration Due to a Relativistic Cosmological Model More Complex than FLRW?
• Detecting Cosmic Strings in the CMB with the Canny Algorithm
• Origin of holographic dark energy models
• Do observations prove that cosmological neutrinos are thermally distributed?
• A large sample of low surface brightness disk galaxies from the SDSS. I: The sample and the stellar populations
• A Hubble diagram from Type II Supernovae based solely on photometry: the Photometric-Colour Method
• VSA Observations of the Anomalous Microwave Emission in the Perseus Region
• Theoretical tools for CMB physics
• Formation of voids in the Universe within the Lemaitre-Tolman model
• Interacting Energy Components and Observational $H(z)$ Data
• Nonlinear evolution of dark matter and dark energy in the Chaplygin-gas cosmology
• The early stage of a cosmic collision? XMM-Newton unveils two obscured AGN in the galaxy pair ESO509-IG066
• The generalized second law in irreversible thermodynamics for the interacting dark energy in a non-flat FRW universe enclosed by the apparent horizon
• CMB anisotropy power spectrum using linear combinations of WMAP maps
• Holographic dark energy in Brans-Dicke theory with log correction
• Interacting entropy-corrected new agegraphic dark energy in Brans-Dicke cosmology
• Effects of Electromagnetic Field on the Dynamics of Bianchi type $V{I}_0$ Universe with Anisotropic Dark Energy
• An inflation model with large variations in spectral index
• Measuring our universe from galaxy redshift surveys
• Sparse component separation for accurate CMB map estimation
• Probing the Evolution of the Galaxy Interaction/Merger Rate Using Collisional Ring Galaxies
• Constraining Born-Infeld models of dark energy with CMB anisotropies
• Constraining Fundamental Physics with Future CMB Experiments
• Probing the Reionization History Using the Spectra of High-Redshift Sources
• Fast spin +-2 spherical harmonics transforms and application in cosmology
• Observational Constraints on Monomial Warm Inflation
• Unveiling the nature of the highly obscured AGN in NGC5643 with XMM-Newton
• Microwave sky and the local Rees-Sciama effect
• Higgs Mass Bounds, Type II SeeSaw and LHC
• Correspondence between DBI-essence and Modified Chaplygin Gas and the Generalized Second Law of Thermodynamics
• Origins Space Telescope Mission Concept Study Report
• A maximum likelihood approach to the destriping technique
• Constraints on primordial isocurvature perturbations and spatial curvature by Bayesian model selection
• Tests of the CMB temperature-redshift relation, CMB spectral distortions and why adiabatic photon production is hard
• LHC discovery potential of the lightest NMSSM Higgs in the h1 -> a1 a1 -> 4 muons channel
• First measurement of the bulk flow of nearby galaxies using the cosmic microwave background
• New light on Dark Cosmos
• Energy-Momentum Tensor of Cosmological Fluctuations during Inflation
• Suppressing the impact of a high tensor-to-scalar ratio on the temperature anisotropies
• Wormhole supported by dark energy admitting conformal motion
• Eternal Inflation with alpha'-Corrections
• Estimating the spectral indices of correlated astrophysical foregrounds by a second-order statistical approach
• Hyperbolic Universes with a Horned Topology and the CMB Anisotropy
• The Effects of Gravitational Back-Reaction on Cosmological Perturbations
• Thermal Effects on Pure and Hybrid Inflation
• Generalized second law of thermodynamics for a phantom energy accreting BTZ black hole
• Searching for Star Formation Beyond Reionization
• Teleparallel dark energy model with a fermionic field via Noether symmetry
• Inflationary Perturbations from Deformed CFT
• Stability of de Sitter spacetime under isotropic perturbations in semiclassical gravity
• Microwave Background Correlations from Dipole Anisotropy Modulation
• Coincidence Problem in YM Field Dark Energy Model
• Canny Algorithm, Cosmic Strings and the Cosmic Microwave Background
• Quantum noise and large-scale cosmic microwave background anisotropy
• Boltzmann hierarchy for the cosmic microwave background at second order including photon polarization
• On B_s -> mu+ mu- and Cold Dark Matter Scattering in the MSSM with Non-Universal Higgs Masses
• From Young and Hot to Old and Cold: Comparing White Dwarf Cooling Theory to Main Sequence Stellar Evolution in Open Clusters
• Massive relic gravitational waves from f(R) theories of gravity: production and potential detection
• A new analysis of Poincaré dodecahedral space model
• CMB and foregrounds in WMAP first year data
• Non-minimally Coupled Tachyonic Inflation in Warped String Background
• Anisotropic Universe Models in Brans-Dicke Theory
• Luminosity distance and redshift in the Szekeres inhomogeneous cosmological models
• Interacting entropy-corrected new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• Inflationary potentials yielding constant scalar perturbation spectral indices
• Anomalous CMB north-south asymmetry
• Sandage-Loeb test for the new agegraphic and Ricci dark energy models
• Casimir Effect confronts Cosmological Constant
• Polarization Observations of the Anomalous Microwave Emission in the Perseus Molecular Complex with the Cosmosomas Experiment
• Scanning strategy for mapping the Cosmic Microwave Background anisotropies with Planck
• What is the best way to measure baryonic acoustic oscillations?
• Post-starburst--AGN Connection: Spatially Resolved Spectroscopy of Hdelta-Strong AGNs
• CBI limits on 31 GHz excess emission in southern HII regions
• One-loop f(R) Gravitational Modified Models
• Uncertainties of Cosmic Ray Spectra and Detectability of Antiproton mSUGRA Contributions With PAMELA
• Supernova constraints on alternative models to dark energy
• Phenomenological Indications of the Scale of Supersymmetry
• Anisotropic brane gravity with a confining potential
• Planck constraints on scalar-tensor cosmology and the variation of the gravitational constant
• The Luminosity Functions of the Galaxy Cluster MS1054-0321 at z=0.83 based on ACS Photometry
• A Note on Gravitational Baryogenesis
• Observational Constraints on Modified Chaplygin Gas from Cosmic Growth
• Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in non-flat universe
• Stochastic Homology of Gaussian vs. non-Gaussian Random Fields: Graphs towards Betti Numbers and Persistence Diagrams
• The transient acceleration from time-dependent interacting dark energy models
• Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
• Dark energy model with variable $q$ and $\omega$ in LRS Bianchi-II space-time
• Moduli Instability in Warped Compactifications of the Type IIB Supergravity
• Oscillons in Scalar Field Theories: Applications in Higher Dimensions and Inflation
• Moduli Stabilisation and Applications in IIB String Theory
• Effect of Vacuum Energy on Evolution of Primordial Black Holes in Einstein Gravity
• The Effective Theory of Inflation in the Standard Model of the Universe and the CMB+LSS data analysis
• Observational constraints on dark energy model
• The Apparent (Gravitational) Horizon in Cosmology
• Examining the Effect of the Map-Making Algorithm on Observed Power Asymmetry in WMAP Data
• Tideless Traversable Wormholes surrounded by cloud of strings in $f(R)$ gravity
• Boundary Effective Field Theory and Trans-Planckian Perturbations: Astrophysical Implications
• Cyclic and heteroclinic flows near general static spherically symmetric black holes
• Precision of Inflaton Potential Reconstruction from CMB Using the General Slow-Roll Approximation
• Attractors, Statefinders and Observational Measurement for Chameleonic Brans--Dicke Cosmology
• Maximum Entropy for Gravitational Wave Data Analysis: Inferring the Physical Parameters of Core-Collapse Supernovae
• Multiple-field inflation and the CMB
• Antiproton-to-Proton Ratios for ALICE Heavy-Ion Collisions
• The environment of Low Surface Brightness Galaxies
• Warm Anisotropic Inflationary Universe Model
• Dust and Ionized Gas in Nine Nearby Early-Type Galaxies Imaged with the HST Advanced Camera for Surveys
• Probing decisive answers to dark energy questions from cosmic complementarity and lensing tomography
• Power Suppression at Large Scales in String Inflation
• Hubble Space Telescope Observations of Nine High-Redshift ESSENCE Supernovae
• Dark energy with polytropic equation of state
• Looking for a Heavy Higgsino LSP in Collider and Dark Matter Experiments
• Searching for Cosmic Strings in New Observational Windows
• The Primordial Perturbation Spectrum from Various Expanding and Contracting Phases
• Cosmic Strings
• Improved Bounds on Universal Extra Dimensions and Consequences for LKP Dark Matter
• Quantum FRW cosmological solutions in the presence of Chaplygin gas and perfect fluid
• Role of the Brans-Dicke scalar in the holographic description of dark energy
• Power-law solutions in $f(T)$ gravity
• Cosmological neutrinos
• Testing Cosmology with Cosmic Sound Waves
• Cosmological non-Gaussian Signature Detection: Comparing Performance of Different Statistical Tests
• Probing dark energy with steerable wavelets through correlation of WMAP and NVSS local morphological measures
• SUSY-GUTs, SUSY-Seesaw and the Neutralino Dark Matter
• Have Atmospheric Cerenkov Telescopes Observed Dark Matter?
• $f(R,T)=f(R)+\lambda T$ gravity models as alternatives to cosmic acceleration
• Noncommutative models in patch cosmology
• Feynman-Weinberg Quantum Gravity and the Extended Standard Model as a Theory of Everything
• WMAP constraints on the Intra-Cluster Medium
• The distance to Hydra and Centaurus from surface brightness fluctuations: Consequences for the Great Attractor model
• Does a black hole rotate in Chern-Simons modified gravity?
• WMAP 3-year primordial power spectrum
• Limits on primordial non-Gaussianities from BOSS galaxy-clustering data
• VLBA Polarization Observations of Markarian 421 After a Gamma-Ray High State
• Noise in strong lensing cosmography
• Loop Quantum Cosmology Gravitational Baryogenesis
• Model-independent cosmological constraints from growth and expansion
• Covariance of CMB anomalies
• Smooth hybrid inflation in supergravity with a running spectral index and early star formation
• Entanglement from thermal black body radiation
• Accessibility of the Pre-Big-Bang Models to LIGO
• Adiabatic compression and indirect detection of supersymmetric dark matter
• Constraints on the Polarization of the Anomalous Microwave Emission in the Perseus Molecular Complex from 7-year WMAP data
• Prospects for Sparticle Discovery in Variants of the MSSM
• Likelihood methods for the combined analysis of CMB temperature and polarisation power spectra
• Hidden past of dark energy cosmological models
• Combining WMAP and SDSS Quasar Data on Reionization Constrains Cosmological Parameters and the Star Formation Efficiency
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• A Last Look at the Microwave Haze/Bubbles with WMAP
• Neutralino dark matter in brane world cosmology
• Missing Power vs low-l Alignments in the Cosmic Microwave Background: No Correlation in the Standard Cosmological Model
• Cosmic coincidence problem and variable constants of physics
• Anomalous variance in the WMAP data and Galactic Foreground residuals
• The inner structure of Zeldovich' pancakes
• Theoretical Uncertainties in Inflationary Predictions
• More evidence in favour of Light Dark Matter particles?
• Curvaton reheating in tachyonic inflationary models
• Spitzer characterisation of dust in an anomalous emission region: the Perseus cloud
• Is there a need and another way to measure the Cosmic Microwave Background temperature more accurately?
• Pre-recombinational energy release and narrow features in the CMB spectrum
• The Majorana neutrino masses, neutrinoless double beta decay and nuclear matrix elements
• Cross-correlation of the CMB and foregrounds phases derived from the WMAP data
• On Wormholes supported by phantom energy
• Energy conditions in $f(T)$ gravity with non-minimal torsion-matter coupling
• Braneworld inflation
• Band-power reconstruction of the primordial fluctuation spectrum by the maximum likelihood reconstruction method
• Galaxy Counts on the CMB Cold Spot
• Bianchi Type-I Universe with Wet Dark Fluid
• On the Nature of the Heat Source for Damped Lya Systems
• Accelerating dark energy models with anisotropic fluid in Bianchi type-$V{I}_0$ space-time
• Cosmological perturbations and the reionization epoch
• Energy Conditions in $f(G)$ Modified Gravity with Non-minimal Coupling to Matter
• Edge Detection, Cosmic Strings and the South Pole Telescope
• Brane assisted quintessential inflation with transient acceleration
• Testing Gaussian random hypothesis with the cosmic microwave background temperature anisotropies in the three-year WMAP data
• Stability of Anisotropic Stellar Filaments
• Dynamical effects of the scale invariance of the empty space: The fall of dark matter ?
• Chandra and Far Ultraviolet Spectroscopic Explorer Observations of z~0 Warm-Hot Gas Toward PKS 2155-304
• Blind component separation in wavelet space. Application to CMB analysis
• Non-zero U_{e3} and TeV-Leptogenesis through A_4 symmetry breaking
• The Impact of Energy Feedback on Quasar Evolution and Black Hole Demographics
• Phenomenology of Dirac Neutrinogenesis in Split Supersymmetry
• The broad-band XMM-Newton and INTEGRAL spectra of bright type 1 Seyfert galaxies
• A Model to Explain Varying $\Lambda$, $G$ and ${\sigma }^2$ Simultaneously
• 3-loop Yang-Mills Condensate Dark Energy Model And Its Cosmological Constraints
• Spectroscopic confirmation of high-redshift supernovae with the ESO VLT
• Detectability of tensor modes in the presence of foregrounds
• Constraints on Evolutionary Properties of GHz Peaked Spectrum Galaxies
• Inflation parameters from Gauss-Bonnet braneworld
• Occam's razor meets WMAP
• Testing a direction-dependent primordial power spectrum with observations of the Cosmic Microwave Background
• Lepton Flavor Violating Decays, Soft Leptogenesis and SUSY SO(10)
• Chandra View of the Warm-Hot IGM toward 1ES 1553+113: Absorption Line Detections and Identifications (Paper I)
• A Note on Curvature Fluctuation of Noncommutative Inflation
• Leptonic CP Violation and Neutrino Mass Models
• A First Glimpse of String Theory in the Sky?
• Measuring the 2D Baryon Acoustic Oscillation signal of galaxies in WiggleZ: Cosmological constraints
• Relic density of neutralino dark matter in the MSSM with CP violation
• The joint large-scale foreground-CMB posteriors of the 3-year WMAP data
• Non-minimal Maxwell-Modified Gauss-Bonnet Cosmologies: Inflation and Dark Energy
• On Anisotropic Dark Energy
• Fermion polarization in sfermion decays as a probe of CP phases in the MSSM
• Potential and mass-matrix in gauged N=4 supergravity
• The cut-sky cosmic microwave background is not anomalous
• Model-independent dark energy test with sigma_8 using results from the Wilkinson Microwave Anisotropy Probe
• Constraining the Primordial Magnetic Field from Cosmic Microwave Background Anisotropies at Higher Multipoles
• Probing the CP-violating light neutral Higgs in the charged Higgs decay at the LHC
• Light Deflection, Lensing, and Time Delays from Gravitational Potentials and Fermat's Principle in the Presence of a Cosmological Constant
• Crossing of the w=-1 Barrier in Two-Fluid Viscous Modified Gravity
• Implications of the B-mode Polarization Measurement for Direct Detection of Inflationary Gravitational Waves
• Some remarks about non-minimally coupled scalar field models
• Detecting Sunyaev-Zel'dovich clusters with PLANCK: II. Foreground components and optimised filtering schemes
• Backreaction from non-conformal quantum fields in de Sitter spacetime
• Dark energy and dark matter from cosmological observations
• Exploring the Systematic Uncertainties of Type Ia Supernovae as Cosmological Probes
• Microwave-Sky Simulations and Projections for Galaxy Cluster Detection with the Atacama Cosmology Telescope
• Directional dependence of CMB parity asymmetry
• Effects of Inhomogeneities on Cosmic Expansion
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• Standard Cosmological Evolution in a Wide Range of f(R) Models
• Large-scale power in the CMB and new physics: an analysis using Bayesian model comparison
• New Agegraphic Dark Energy in $f(R)$ Gravity
• Gauge vs. Gravity mediation in models with anomalous U(1)'s
• Transitioning Universe with hybrid scalar field in Bianchi I space-time
• Impact of Galactic polarized emission on B-mode detection at low multipoles
• Fluctuations of cosmological birefringence and the effect on CMB B-mode polarization
• Running Spectral Index as a Probe of Physics at High Scales
• Complex data processing: fast wavelet analysis on the sphere
• Lepton Flavour Violating Leptonic/Semileptonic Decays of Charged Leptons in the Minimal Supersymmetric Standard Model
• Do star formation rates of galaxy clusters depend on mass?: blue/late-type fractions, total star formation rates of 115 galaxy clusters as a function of cluster virial mass
• Second-order gravitational effects of local inhomogeneities on CMB anisotropies and non-Gaussian signatures
• On the Presence of Thermal SZ Induced Signal in the First Year WMAP Temperature Maps
• Mechanics and Newton-Cartan-Like Gravity on the Newton-Hooke Space-time
• From Primordial Quantum Fluctuations to the Anisotropies of the Cosmic Microwave Background Radiation
• Diagnostic Potential of Cosmic-Neutrino Absorption Spectroscopy
• Stochastic chemical enrichment in metal-poor systems I. Theory
• Cosmic acceleration and crossing of $\omega =-1$ in non-minimal modified Gauss-Bonnet gravity
• Quintessence From The Decay of a Superheavy Dark Matter
• Flat rotation curves in Chern-Simons modified gravity
• Testing Fractional Action Cosmology
• Accounting for the time evolution of the equation of state parameter during reheating
• Thermodynamics of viscous dark energy in an RSII braneworld
• Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
• Bounce cosmology in $f(\mathcal{R})$ gravity
• Minimal Theoretical Uncertainties in Inflationary Predictions
• Aspects of Quantum Gravity in de Sitter Spaces
• Primordial non-Gaussianity: local curvature method and statistical significance of constraints on f_NL from WMAP data
• CMB Lensing and the WMAP Cold Spot
• Phantom Energy Accretion by Stringy Charged Black Hole
• Stability analysis and Observational Measurement in Chameleonic Generalised Brans--Dicke Cosmology
• Top-Down Fragmentation of a Warm Dark Matter Filament
• Can a primordial magnetic field originate large-scale anomalies in WMAP data?
• Planck intermediate results. VII. Statistical properties of infrared and radio extragalactic sources from the Planck Early Release Compact Source Catalogue at frequencies between 100 and 857 GHz
• Generalized Gravitational Baryogenesis of Well-Known $f(T,T_G)$ and $f(T,B)$ Models
• A Scaling Index Analysis of the WMAP three year data: Signatures of non-Gaussianities and Asymmetries in the CMB
• Interacting new agegraphic viscous dark energy with varying $G$
• Nonlinear Evolution of Cosmic Magnetic Fields and Cosmic Microwave Background Anisotropies
• Minimal seesaw model with tri/bi-maximal mixing and leptogenesis
• Deep GMRT 150 MHz observations of the LBDS-Lynx region: Ultra-Steep Spectrum Radio Sources
• The galaxy cluster Ysz-Lx and Ysz-M relations from the WMAP 5-yr data
• Second-order Gauge-invariant Cosmological Perturbation Theory: Current Status
• Can Planck-scale physics be seen in the cosmic microwave background ?
• Wormhole solutions with a polynomial equation-of-state and minimal violation of the null energy condition
• Holographic Dark Energy Models and Higher Order Generalizations in Dynamical Chern-Simons Modified Gravity
• Imprints of spherical non-trivial topologies on the CMB
• Statistics of phase correlations as a test for non-Gaussianity of the CMB maps
• The accelerating universe and a limiting curvature proposal
• Revisiting the Constraint on the Helium Abundance from CMB
• The covariance of cosmic shear correlation functions and cosmological parameter estimates using redshift information
• An upper limit to polarized submillimetre emission in Arp 220
• Cosmic Behavior, Statefinder Diagnostic and $w-w^{\prime }$ Analysis for Interacting NADE model in Non-flat Universe
• Preheating after N-flation
• Anisotropy of the galaxy cluster X-ray luminosity-temperature relation
• The Yuan-Tseh Lee Array for Microwave Background Anisotropy
• Can Holographic dark energy models fit the observational data?
• The coincidence problem in linear dark energy models
• The supersymmetric interpretation of the EGRET excess of diffuse Galactic gamma rays
• Exotic solutions in General Relativity: Traversable wormholes and 'warp drive' spacetimes
• Statefinder Parameters for Interacting Phantom Energy with Dark Matter
• Accelerating universe in $f(\mathcal{R})$ brane gravity
• Implications of a new temperature scale for halo dwarfs on LiBeB and chemical evolution
• A Markov Chain Monte Carlo Algorithm for analysis of low signal-to-noise CMB data
• Cross-Calibration of Cluster Mass-Observables
• Sensitivity of Supersymmetric Dark Matter to the b Quark Mass
• Five-dimensional generalized $f(R)$ gravity with curvature-matter coupling
• DGP Cosmology with a Non-Minimally Coupled Scalar Field on the Brane
• Systematic corrections to the measured cosmological constant as a result of local inhomogeneity
• Primordial Neutrinos, Cosmological Perturbations in Interacting Dark-Energy Model: CMB and LSS
• COSMOSOMAS Observations of the CMB and Galactic Foregrounds at 11 GHz: Evidence for anomalous microwave emission at high Galactic Latitude
• Probing the Universe on Gigaparsec Scales with Remote Cosmic Microwave Background Quadrupole Measurements
• Inflationary power asymmetry from primordial domain walls
• Performance forecasts for the primordial gravitational wave detection pipelines for AliCPT-1
• Holographic dark energy in a non-flat universe with Granda-Oliveros cut-off
• Weak lensing signal in Unified Dark Matter models
• Dynamical Evolution of Interacting Modified Chaplygin Gas
• Upper Limits on the Extragalactic Background Light from the Gamma-Ray Spectra of Blazars
• Density inhomogeneities in heavy ion collisions around the critical point
• The running-mass inflation model and WMAP
• Constraining Warm Inflation with the Cosmic Microwave Background
• Determining the equation of state of dark energy from angular size of compact radio sources and X-ray gas mass fraction of galaxy clusters
• Absence of isentropic expansion in various inflation models
• The Mass, Baryonic Fraction, and X-ray Temperature of the Luminous, High Redshift Cluster of Galaxies, MS0451.6-0305
• Triple Experiment Spectrum of the Sunyaev-Zeldovich Effect in the Coma Cluster: H_0
• Dynamical Collapse of Charged Scalar Field in Phantom Gravity
• Observational biases in Lagrangian reconstructions of cosmic velocity fields
• Equilibrium hydrostatic equation and Newtonian limit of the singular f(R) gravity
• A Statistical Analysis of Intergalactic Medium Transmission Approaching Reionization
• Observational constraints on cosmic strings: Bayesian analysis in a three dimensional parameter space
• Dating the stellar population in massive early-type galaxies at $z\sim$1.5
• Effects of inhomogeneities on apparent cosmological observables: "fake" evolving dark energy
• Contribution of the QCD $\Theta$-term to nucleon electric dipole moment
• An upper limit on anomalous dust emission at 31 GHz in the diffuse cloud [LPH96]201.663+1.643
• Abundance diagnosis of E+A (post-starburst) galaxies
• Coupling Quintessence to Inflation in Supergravity
• Cosmological parameters and the WMAP data revisited
• Cosmic Dynamics in the Chameleon Cosmology
• Non-linear perturbations in scalar-tensor cosmologies
• Non-Gaussianity in the WMAP data using the peak-peak correlation function
• Testing gaussianity, homogeneity and isotropy with the cosmic microwave background
• Long-term variability of extragalactic radio sources in the Planck Early Release Compact Source Catalogue
• Preheating curvature perturbations with a coupled curvaton
• Constraints on extended quintessence from high-redshift Supernovae
• Reconstruction of the primordial fluctuation spectrum from the five-year WMAP data by the cosmic inversion method with band-power decorrelation analysis
• Supernova tests of the timescape cosmology
• Clarifying Inflation Models: Slow-roll as an expansion in 1/N_{efolds}
• Primordial magnetic fields and gravitational baryogenesis in nonlinear electrodynamics
• Effects of thermohaline instability and rotation-induced mixing on the evolution of light elements in the Galaxy : D, 3He and 4He
• Cosmic age, Statefinder and $Om$ diagnostics in the decaying vacuum cosmology
• Baryon Number Violating Scalar Diquarks at the LHC
• Accelerating cosmologies from compactification with a twist
• Inflation With Realistic Supersymmetric SO(10)
• Joining the Hubble Flow: Implications for Expanding Space
• Radion Cosmology in Theories with Universal Extra Dimensions
• Neutralino-Nucleon Cross Section and Charge and Colour Breaking Constraints
• No evidence for the cold spot in the NVSS radio survey
• Footprints of Statistical Anisotropies
• Constraining Cosmological Parameters by the Cosmic Inversion Method
• Generalized holographic dark energy model described at the Hubble length
• Observational constraints on generalized Chaplygin gas model
• Optical Polarimetry of the Jets of Nearby Radio Galaxies: I. The Data
• Properties and use of CMB power spectrum likelihoods
• Two-fluid atmosphere from decelerating to accelerating FRW dark energy models
• SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
• Dark viscous fluid described by a unified equation of state in cosmology
• Constraining Extended Theories of Gravity using Solar System Tests
• Statefinder diagnostic and $w-w^{\prime }$ analysis for interacting polytropic gas dark energy model
• Primordial Power Spectrum Reconstruction
• Formation and evolution of early-type galaxies. II. Models with quasi-cosmological initial conditions
• Do We Have Evidence for New Physics in the Sky?
• LTB universes as alternatives to dark energy: does positive averaged acceleration imply positive cosmic acceleration?
• Linearized Bekenstein Varying Alpha Models
• Equation of state for Universe from similarity symmetries
• Element segregation in giant galaxies and X-ray clusters
• Constraints on Singular Evolution from Gravitational Baryogenesis
• Effects of quantum gravity on the inflationary parameters and thermodynamics of the early universe
• Low Energy Effective Action for Dilatonic Braneworld --A Formalism for Inflationary Braneworld--
• Relic gravitational waves from Quintessential Inflation
• Evidence for the Missing Baryons in the Angular Correlation of the Diffuse X-ray Background
• Unexpected Topology of the Temperature Fluctuations in the Cosmic Microwave Background
• Phantom Accretion onto the Schwarzschild de-Sitter Black Hole
• Holographic dark energy in Brans-Dicke cosmology with Granda-Oliveros cut-off
• Nonparametric Inference for the Cosmic Microwave Background
• Modeling and replicating statistical topology, and evidence for CMB non-homogeneity
• Constraining Inflation
• Did WMAP see Moving Local Structures?
• A Robust Measure of Cosmic Structure beyond the Power-Spectrum: Cosmic Filaments and the Temperature of Dark Matter
• Lepton Flavor Violation in Extra Dimension Models
• Accretion of Phantom Energy and Generalized Second Law of Thermodynamics for Einstein-Maxwell-Gauss-Bonnet Black Hole
• On the Higgs Mass in the CMSSM
• Cosmic microwave background snapshots: pre-WMAP and post-WMAP
• 21 cm intensity mapping with the Five hundred metre Aperture Spherical Telescope
• Modeling Transit Dark Energy in $f(R,L_m)$-gravity
• Confronting the Hubble Diagram of Gamma-Ray Bursts with Cardassian Cosmology
• The integrated bispectrum as a test of CMB non-Gaussianity: detection power and limits on f_NL with WMAP data
• Aberration of the Cosmic Microwave Background
• Reconstructing the Primordial Spectrum with CMB Temperature and Polarization
• Using Multipoles of the Correlation Function to Measure H(z), D_A(z), and β(z) from Sloan Digital Sky Survey Luminous Red Galaxies
• Reconstruction of modified gravity with ghost dark energy models
• A VSA search for the extended Sunyaev-Zel'dovich Effect in the Corona Borealis Supercluster
• Cosmological Perturbations on a Bouncing Brane
• Crossing of $\omega =-1$ with Tachyon and Non-minimal Derivative Coupling
• Optical and Near-Infrared Observations of the Peculiar Type Ia Supernova 1999ac
• Genus Topology of the Cosmic Microwave Background from the WMAP 3-Year Data
• Direct Wavelet Expansion of the Primordial Power Spectrum
• Cosmography with next-generation gravitational wave detectors
• CMB Polarimetry using Correlation Receivers with the PIQUE and CAPMAP Experiments
• Inhomogeneous Big Bang Nucleosynthesis Revisited
• Anomalous radio emission from dust in the Helix
• An alpha-stable approach to the study of the P(D) distribution of unresolved point sources in CMB sky maps
• Bianchi Type $I$ Cosmology in $f(R,T)$ Gravity
• C-Band All-Sky Survey: A First Look at the Galaxy
• Multiple kinetic k-essence, phantom barrier crossing and stability
• Cardassian Expansion: Dark Energy Density from Modified Friedmann Equations
• Primordial Molecular Emission in Population III Galaxies
• Accretion Properties of A Sample of Hard X-ray (<60keV) Selected Seyfert 1 Galaxies
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Effects of Anisotropy on the Sign-Changeable Interacting Tsallis Holographic Dark Energy
• Semi-analytical approach to magnetized temperature autocorrelations
• Testing the DGP model with gravitational lensing statistics
• Phantom energy accretion onto a black hole in Horava Lifshitz gravity
• A redshift survey towards the CMB Cold Spot
• Anisotropic universe with anisotropic sources
• Patterns of Lepton-Flavour Violation Motivated by Decoupling and Sneutrino Inflation
• Temperature Fluctuations of the Cosmic Microwave Background Radiation: A Case of Nonextensivity?
• Galaxy clustering constraints on deviations from Newtonian gravity at cosmological scales II: Perturbative and numerical analyses of power spectrum and bispectrum
• A Comparison of Cosmological Models Using Strong Gravitational Lensing Galaxies
• CMB Constraints on Principal Components of the Inflaton Potential
• Is There an Imprint of Primordial Stars in the Tev Gamma-Ray Spectrum of Blazars?
• Statefinder diagnosis and the interacting ghost model of dark energy
• The circles-in-the-sky signature for three spherical universes
• Cosmological perturbations and noncommutative tachyon inflation
• Heavy Element Production in Inhomogeneous Big Bang Nucleosynthesis
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• Supersymmetry on the Run: LHC and Dark Matter
• An Observational Pursuit for Population III Stars in a Ly_alpha Emitter at z=6.33 through HeII Emission
• Brans-Dicke Scalar Field Cosmological Model in Lyra's Geometry
• Corrections to the apparent value of the cosmological constant due to local inhomogeneities
• An exploration of an early gravity transition in light of cosmological tensions
• Asymptotically flat wormhole solutions with variable equation-of-state parameter
• Current experimental constraints on NMSSM with large lambda
• Scalar field "mini--MACHOs": a new explanation for galactic dark matter
• Tachyonic Inflation in a Warped String Background
• Needlet Bispectrum Asymmetries in the WMAP 5-year Data
• Statistical challenges in the analysis of Cosmic Microwave Background radiation
• AMiBA: Broadband Heterodyne CMB Interferometry
• Reconstructing Sunyaev-Zeldovich clusters in future CMB experiments
• Studying Type II supernovae as cosmological standard candles using the Dark Energy Survey
• Probing Inflation and Dark Energy with Current Cosmological Observations
• Cosmological viability conditions for $f(T)$ dark energy models
• The intrinsic B-mode polarisation of the Cosmic Microwave Background
• Linearization of homogeneous, nearly-isotropic cosmological models
• Broadband X-Ray Observations of the 2018 Outburst of the Changing-Look Active Galactic Nucleus NGC 1566
• Cosmic nucleosynthesis: a multi-messenger challenge
• On Principle of Inertia in Closed Universe
• Dumping inflaton energy density out of this world
• The power spectrum amplitude from clusters revisited: σ_8 using simulations with preheating and cooling
• Accelerating Bianchi Type-V Cosmology with Perfect Fluid and Heat Flow in Saez-Ballester Theory
• Extended quintessence, inflation, and stable de Sitter spaces
• Perspectives for the detection and measurement of Supersymmetry in the focus point region of mSUGRA models with the ATLAS detector at LHC
• Beam mismatch effects in Cosmic Microwave Background polarization measurements
• Tolman IV fluid sphere in f(R, T) gravity
• Cross-Correlation Studies between CMB Temperature Anisotropies and 21 cm Fluctuations
• Thermodynamics in Closed Universe with Entropy Corrections
• Compressed sensing reconstruction of a string signal from interferometric observations of the cosmic microwave background
• Universal Signature of Non-Quantum Systems
• Temperature at Horizon in de Sitter Spacetime
• Planck-Scale Effects on Global Symmetries: Cosmology of Pseudo-Goldstone Bosons
• Power Spectrum of Cosmic Momentum Field Measured from the SFI Galaxy Sample
• The millimeter-wave continuum spectrum of Centaurus A and its nucleus
• SUSY dark matter in light of CDMS II results: a comparative study for different models
• Simulations of the Sunyaev-Zeldovich Effect from Quasars
• Doppler boosting the stochastic gravitational wave background
• Stochastic background of relic scalar gravitational waves from scalar-tensor gravity
• $\mu -\tau$ Symmetry and Radiatively Generated Leptogenesis
• Why Does Gravity Ignore the Vacuum Energy?
• Cosmological Structure Formation Creates Large-Scale Magnetic Fields
• Directional dependence of LCDM cosmological parameters
• Archeops In-flight Performance, Data Processing and Map Making
• A Theory of a Spot
• Quadrupole--octopole alignment of CMB related to primordial power spectrum with dipolar modulation in anisotropic spacetime
• Investigating the origins of the CMB-XRB cross correlation
• Reconstructing the history of dark energy using maximum entropy
• Did Boomerang hit MOND?
• The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity
• Baryogenesis in $f(R,L_m)$ gravity
• Constraining $f(T,\mathcal{T})$ Gravity with Gravitational Baryogenesis
• Some Impacts of Lorentz Violation on Cosmology
• Statefinder diagnostic for Yang-Mills dark energy model
• General Slow-Roll Spectrum for Gravitational Waves
• Agegraphic Chaplygin gas model of dark energy
• Foreground Analysis Using Cross-Correlations of External Templates on the 7-year WMAP data
• Phantom Wormhole Solutions in a Generic Cosmological Constant Background
• A new approach in stability analysis: case study: tachyon cosmology with non-minimally coupled scalar field-matter
• Large-Scale Non-Gaussianities in the 21 cm Background Anisotropies From the Era of Reionization
• Fractional-order derivatives in cosmological models of accelerated expansion
• A mathematical analysis of the evolution of perturbations in a modified Chaplygin gas model
• Phenomenology of a Fluxed MSSM
• Mixed Higgsino Dark Matter from a Reduced SU(3) Gaugino Mass: Consequences for Dark Matter and Collider Searches
• CMB Alignment in Multi-Connected Universes
• Non-Random Phases in Non-Trivial Topologies
• KiDS-SBI: Simulation-based inference analysis of KiDS-1000 cosmic shear
• Groups in the Millennium Simulation and in SDSS DR7
• Reconstructing interacting new agegraphic polytropic gas model in non-flat FRW universe
• Cosmological influence of super-Hubble perturbations
• CMB signal in WMAP 3yr data with FastICA
• Hologrphy and holographic dark energy model
• E+A and Companion Galaxies - I : A Catalogue and Statistics
• High-Energy Constraints on the Direct Detection of MSSM Neutralinos
• Cosmographic analysis of a closed bouncing universe with the varying cosmological constant in $f(R,T)$ gravity
• Neutralino Dark Matter from MSSM Flat Directions in light of WMAP Result
• CMB Temperature and Matter Power Spectrum in a Decay Vacuum Dark Energy Model
• Perturbative approach for mass varying neutrinos coupled to the dark sector in the generalized Chaplygin gas scenario
• Why Cosmic Voids Matter: Nonlinear Structure & Linear Dynamics
• Fe II Diagnostic Tools for Quasars
• Do Observations Favour Galileon Over Quintessence?
• Kaluza-Klein Dark Matter, Electrons and Gamma Ray Telescopes
• Type II Seesaw and the PAMELA/ATIC Signals
• A direct link between neutrinoless double beta decay and leptogenesis in a seesaw model with $S_4$ symmetry
• Efficient Coannihilation Process through Strong Higgs Self-Coupling in LKP Dark Matter Annihilation
• Basics of inflationary cosmology
• Bayesian analysis of anisotropic cosmologies: Bianchi VII_h and WMAP
• Deceleration from Entrainment in the jet of the quasar 1136-135?
• How binary interactions affect spectral stellar population synthesis
• Dark Energy Interacting with Dark Matter in Classical Einstein and Loop Quantum Cosmology
• Sunyaev-Zel'dovich Effects from Quasars in Galaxies and Groups
• Perturbations of Matter Fields in the Second-order Gauge-invariant Cosmological Perturbation Theory
• Leptogenesis from a sneutrino condensate revisited
• XMM-{\em Newton} and FUSE Tentative Evidence for a WHIM filament along the Line of Sight to PKS~0558-504
• Modular inflation and the orthogonal axion as curvaton
• Relic density and elastic scattering cross sections of the neutralino in the MSSM with CP-violating phases
• Bouncing cosmology in modified gravity with higher-order Gauss-Bonnet curvature term
• Reconstructing generalized ghost condensate model with dynamical dark energy parametrizations and observational datasets
• Can one hear the shape of the Universe?
• Bouncing universe with the non-minimally coupled scaler field and its reconstructing
• BSM Higgs Physics in the Exclusive Forward Proton Mode at the LHC
• Optimal filters on the sphere
• Decaying Superheavy Dark Matter and Subgalactic Structure of the Universe
• Generalized CMB initial conditions with pre-equality magnetic fields
• Constraining Dark Energy by Combining Cluster Counts and Shear-Shear Correlations in a Weak Lensing Survey
• Scenarios of modulated perturbations
• Recent Progress in Search for Dark Sector Signatures
• Snyder's Quantized Space-time and De Sitter Special Relativity
• Splitting the split supersymmetry
• Constraints on standard and non-standard early Universe models from CMB B-mode polarization
• Variable G correction to statefinder parameters of dark energy
• Constraining Cut-off Physics in the Cosmic Microwave Background
• New allowed mSUGRA parameter space from variations of the trilinear scalar coupling A0
• Non-chaotic dynamics in general-relativistic and scalar-tensor cosmology
• Experimental constraints on nMSSM and implications on its phenomenology
• Gravitational energy and cosmic acceleration
• Tau Flavour Violation in Sparticle Decays at the LHC
• Cosmological Density Fluctuations on 100Mpc Scales and their ISW Effect
• Brany Liouville Inflation
• Expansion history and f(R) modified gravity
• Non-Gaussianity analysis on local morphological measures of WMAP data
• Extended Phase Space Analysis of Interacting Dark Energy Models in Loop Quantum Cosmology
• Large N Cosmology
• Rapid build-up of the stellar content in the protocluster core SPT2349$-$56 at $z=4.3$
• Black hole and holographic dark energy
• Observational Constraints with Recent Data on the DGP Modified Gravity
• Tracing the Warm Hot Intergalactic Medium in the local Universe
• Second-Order Corrections to the Power Spectrum in the Slow-Roll Expansion with a Time-Dependent Sound Speed
• Measurability of vacuum fluctuations and dark energy
• Running of Low-Energy Neutrino Masses, Mixing Angles and CP Violation
• Scale-Invariant Fluctuations from Galilean Genesis
• Low Scale Leptogenesis and Dark Matter Candidates in an Extended Seesaw Model
• Undulant Universe
• Interacting viscous ghost tachyon, K-essence and dilaton scalar field models of dark energy
• Constraints on scalar and tensor perturbations in phenomenological and two-field inflation models: Bayesian evidences for primordial isocurvature and tensor modes
• Sub-GeV galactic cosmic-ray antiprotons from primordial black holes in the Randall-Sundrum braneworld
• "Graceful" Old Inflation
• Tracking quintessence: a dynamical systems study
• Does the Second Caustic Ring of Dark Matter Cause the Monoceros Ring of Stars ?
• Prospects for Direct Detection of Inflationary Gravitational Waves by Next Generation Interferometric Detectors
• Anisotropic Galactic Outflows and Enrichment of the Intergalactic Medium. I: Monte Carlo Simulations
• Instability of reconstruction of the low CMB multipoles
• The nature of the torus in the heavily obscured AGN Markarian 3: an X-ray study
• Affleck-Dine Baryogenesis and heavy elements production from Inhomogeneous Big Bang Nucleosynthesis
• Cosmological neutrino bounds for non-cosmologists
• Thermal radiation from Lorentzian traversable wormholes
• A Realistic Particle Physics Dark Energy Model
• No Higher Criticism of the Bianchi Corrected WMAP Data
• Collision of Domain Walls in asymptotically Anti de Sitter spacetime
• Power-law Parameterized Quintessence Model
• Cosmic vacuum energy decay and creation of cosmic matter
• Cosmological Imprints of Pre-Inflationary Particles
• Vacuum and Gravitons of Relic Gravitational Waves, and Regularization of Spectrum and Energy-Momentum Tensor
• The Luminosity Function and Color-Magnitude Diagram of the Globular Cluster M12
• Non-Gaussianity of Large-Scale Cosmic Microwave Background Anisotropies beyond Perturbation Theory
• Accelerated expansion in modified gravity with a Yukawa-like term
• Cosmological perturbation theory, instantaneous gauges and local inertial frames
• Non-Gaussian Signatures in the five-year WMAP data as identified with isotropic scaling indices
• A Gravity Dual of Ultra-slow Roll Inflation
• Trans-Planckian corrections to the primordial spectrum in the infra-red and the ultra-violet
• The study of topology of the universe using multipole vectors
• Single Field Inflation models allowed and ruled out by the three years WMAP data
• Evidence for Dark Matter Annihilation from Galactic Gamma Rays?
• Mirror World and Superstring-Inspired Hidden Sector of the Universe, Dark Matter and Dark Energy
• A Cyclic Universe With Varying Cosmological Constant in $f(R,T)$ gravity
• Leptogenesis from Spin-Gravity Coupling Following Inflation
• Random-Walk Statistics and the Spherical Harmonic Representation of CMB Maps
• The Revival of White Holes as Small Bangs
• High-energy scalarons in R^{2} gravity as a model for Dark Matter in galaxies
• Interacting Two-Fluid Viscous Dark Energy Models In Non-Flat Universe
• Pearson's random walk in the space of the CMB phases: evidence for parity asymmetry
• Observational constraints on decaying vacuum dark energy model
• Planck intermediate results. XII: Diffuse Galactic components in the Gould Belt System
• Studying the Peculiar Velocity Bulk Flow in a Sparse Survey of Type-Ia SNe
• Dark energy interacting with neutrinos and dark matter: a phenomenological theory
• Effects of space-time noncommutativity on the angular power spectrum of the CMB
• Analytic study on backreacting holographic superconductors with dark matter sector
• History of Hydrogen Reionization in the Cold Dark Matter Model
• Conceptual Problems of Inflationary Cosmology and a New Approach to Cosmological Structure Formation
• Constraints on the solid dark universe model
• The CMB Quadrupole in a Polarized Light
• Absolute Calibration of Diffuse Radio Surveys at 45 and 150 MHz
• Inflationary slow-roll formalism and perturbations in the Randall-Sundrum Type II braneworld
• Optimal scan strategies for future CMB satellite experiments
• Stellar Orbit Constraints on Neutralino Annihilation at the Galactic Center
• CMB likelihood approximation by a Gaussianized Blackwell-Rao estimator
• Decaying Dark Matter and the Deficit of Dwarf Haloes
• Black Holes in Bulk Viscous Cosmology
• The Hubble Slow Roll Expansion for Multi Field Inflation
• X-Ray Emission from the Warm Hot Intergalactic Medium
• Hamiltonian Formalism of the de-Sitter Invariant Special Relativity
• A Map of Diffuse Radio Emission at 182 MHz to Enhance Epoch of Reionization Observations in the Southern Hemisphere
• The Cosmological Constant Problem, an Inspiration for New Physics
• The SZ effect contribution to WMAP. A Cross-Correlation between WMAP and ROSAT
• Big Bang nucleosynthesis in scalar tensor gravity: the key problem of the ${}^7$Li abundance
• Crossing the Phantom Divide Line in a DGP-Inspired $F(R,\varphi )$-Gravity
• Cosmological models in $f(T,\mathcal{T})$ gravity and the dynamical system analysis
• Constraining SUSY Dark Matter with the ATLAS Detector at the LHC
• Mysteries on Universe's Largest Observable Scales
• Galactic Center Extinction: Evidence for Metallic Needles in the General Interstellar Medium
• The Shape, Multiplicity, and Evolution of Superclusters in LambdaCDM Cosmology
• Cosmology with nonminimal kinetic coupling and a Higgs-like potential
• Investigating the accelerated expansion of the Universe through updated constraints on viable $f(R)$ models within the metric formalism
• Solving cosmological problem in universal extra dimension models by introducing Dirac neutrino
• Vector field and rotational curves in dark galactic halos
• The nearly flat universe
• Cosmological constraints on a classical limit of quantum gravity
• Consistency equations in Randall-Sundrum cosmology: a test for braneworld inflation
• A Millimeter-Wave Galactic Plane Survey With The BICEP Polarimeter
• Bound on the time variation of the fine structure constant driven by quintessence
• Testing generalized logotropic models with cosmic growth
• Large Slow Roll Parameters in Single Field Inflation
• Cold dark matter in brane cosmology scenario
• Profile Likelihoods in Cosmology: When, Why and How illustrated with $\Lambda$CDM, Massive Neutrinos and Dark Energy
• Scalar-Tensor Teleparallel Gravity With Boundary Term by Noether Symmetries
• On the smallness of the cosmological constant in SUGRA models
• Traversable wormholes with logarithmic shape function in f(R, T) gravity
• Relic abundance of dark matter in universal extra dimension models with right-handed neutrinos
• CMBfit: Rapid WMAP likelihood calculations with normal parameters
• Two-Fluid Dark Energy Models in Bianchi Type-III Universe with Variable Deceleration Parameter
• Thermodynamics and stability of $f(T,B)$ gravity with viscous fluid by observational constraints
• Bulge evolution in face-on spirals and low surface brightness galaxies
• Long-term monitoring of PKS0558-504 with Swift: the disc-corona link
• Efficiency of pseudo-spectrum methods for estimation of Cosmic Microwave Background B-mode power spectrum
• A full sky prediction of the SZ effect from diffuse hot gas in the local universe and the upper limit from the WMAP data
• Neutrino masses and R-parity violation
• Agegraphic Dark Energy Model in Non-Flat Universe: Statefinder Diagnostic and $w-w^{\prime }$ Analysis
• Cosmic infrared background from Population III stars and its effect on spectra of high-z gamma-ray bursts
• Gravitino production from reheating in split supersymmetry
• Unconventional Cosmology
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• Constraining the dark energy dynamics with the cosmic microwave background bispectrum
• LHC String Phenomenology
• Constraining Bianchi type V universe with recent H(z) and BAO observations in Brans-Dicke theory of gravitation
• Stochastic approaches to inflation model building
• Will black holes eventually engulf the universe?
• Can Cosmic Shear Shed Light on Low Cosmic Microwave Background Multipoles?
• Fermionic partner of Quintessence field as candidate for dark matter
• Moving dark energy and the CMB dipole
• A note on the large-angle anisotropies in the WMAP cut-sky maps
• Mimicking the cosmological constant for more than one observable with large scale inhomogeneities
• Thermodynamical description of the interacting new agegraphic dark energy
• Interacting entropy-corrected new agegraphic dark energy in non-flat universe
• Cosmic Dynamics in $F(R,\varphi )$ Gravity
• Wavelet domain Bayesian denoising of string signal in the cosmic microwave background
• String Inspired Quintom Model with Non-minimally Coupled Modified Gravity
• Physics of the cosmic microwave background anisotropy
• Joint constraints on the lepton asymmetry of the Universe and neutrino mass from the Wilkinson Microwave Anisotropy Probe
• Neutrino mass bounds from cosmology
• Joint modeling of the probability distribution and power spectrum of the Lya forest: comparison with observations at z=3
• Coherent Baryogenesis
• Stochastic Quintessence
• Removing the giants and learning from the crowd: a new SZ power spectrum method and revised Compton $y$-map analysis
• Density growth in Kantowski-Sachs cosmologies with cosmological constant
• The age dependence of galaxy clustering
• The generalized second law for the interacting generalized Chaplygin gas model
• Observation number correlation in WMAP data
• Contamination cannot explain the lack of large-scale power in the cosmic microwave background radiation
• The present universe in the Einstein frame, metric-affine R+1/R gravity
• Measuring the Three Point Correlation Function of the Cosmic Microwave Background
• Bipolar Harmonic encoding of CMB correlation patterns
• CMB Tomography: Reconstruction of Adiabatic Primordial Scalar Potential Using Temperature and Polarization Maps
• Physical Parameters for Stable $f(R)$ Models
• Bias in low-multipole CMB reconstructions
• Large-scale magnetic fields, curvature fluctuations and the thermal history of the Universe
• The WMAP normalization of inflationary cosmologies
• CMB power spectrum estimation using noncircular beams
• Gravitational Lensing by Dark Matter Halos with Non-universal Density Profiles
• The Principle of Relativity, Kinematics and Algebraic Relations
• What do very nearly flat detectable cosmic topologies look like?
• Foreground separation using a flexible maximum-entropy algorithm: an application to COBE data
• Vacuum fluctuations in a supersymmetric model in FRW spacetime
• Cosmic magnetic fields from velocity perturbations in the early Universe
• Low-Redshift Cosmic Baryon Fluid on Large Scales and She-Leveque Universal Scaling
• Assessing Consistency Between WMAP 9-year and Planck 2015 Temperature Power Spectra
• Discovery of Strong Lensing by an Elliptical Galaxy at z=0.0345
• Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra
• Can the cosmological constant be mimicked by smooth large-scale inhomogeneities for more than one observable?
• Redshift spherical shell energy in isotropic Universes
• Noether gauge symmetry for the Bianchi type I model in f(T) gravity
• Perturbations of ionization fractions at the cosmological recombination epoch
• The phenomenology of beyond Horndeski gravity
• A new probe of Axion-Like Particles: CMB polarization distortions due to cluster magnetic fields
• Fixed points and FLRW cosmologies: Flat case
• Cosmic Microwave Background Polarisation: foreground contrast and component separation
• Neutrino number asymmetry and cosmological birefringence
• Density fluctuations in one-field inflation
• Scaling ansatz, four zero Yukawa textures and large ${\theta }_{13}$
• Big-Bang nucleosynthyesis: constraints on nuclear reaction rates, neutrino degeneracy, inhomogeneous and Brans-Dicke models
• Thermodynamics of phantom energy in the presence of a Reissner-Nordstrom black hole
• Scale dependent non-Gaussianities in the CMB data identified with Minkowski Functionals and Scaling Indices
• The hybrid SZ power spectrum: Combining cluster counts and SZ fluctuations to probe gas physics
• Gamma rays from the neutralino dark matter annihilations in the Milky Way substructures
• The Halo, Hot Spots and Jet/Cloud Interaction of PKS 2153--69
• Warped Strings: Self-dual Flux and Contemporary Compactifications
• Bouncing Universe and phantom crossing in Modified Gravity and its reconstruction
• Cosmography and large scale structure by f(R) gravity: new results
• Can the initial singularity be detected by cosmological tests?
• The 2MASS galaxy angular power spectrum: Probing the galaxy distribution to Gigaparsec scales
• Modified gravity inspired DGP brane cosmology
• A Chandra view of Naked Active Galactic Nuclei
• Self-interacting Scalar Field Trapped in a Randall-Sundrum Braneworld: The Dynamical Systems Perspective
• Gravitational Baryogenesis in Anisotropic Universe
• The PSCz Dipole Revisited
• Noether Symmetries of Some Homogeneous Universe Models in Curvature Corrected Scalar-Tensor Gravity
• Noncommutative Black-Body Radiation: Implications On Cosmic Microwave Background
• Faraday Rotation as a diagnostic of Galactic foreground contamination of CMB maps
• Unified Models of Inflation and Quintessence
• Probing the Light Speed Anisotropy with respect to the Cosmic Microwave Background Radiation Dipole
• Bianchi type VI1 cosmological model with wet dark fluid in scale invariant theory of gravitation
• From the Spectrum to Inflation : An Inverse Formula for the General Slow-Roll Spectrum
• Non-gaussianity in the foreground-reduced CMB maps
• SuperWIMP dark matter scenario in light of WMAP
• Calculable lepton masses, seesaw relations and four neutrino mixings in a 3-3-1 model with extra U(1) symmetry
• Steerable wavelet analysis of CMB structures alignment
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Cosmological gamma ray and neutrino backgrounds due to neutralino dark matter annihilation
• New Constraints on the Variable Equation of State Parameter from X-Ray Gas Mass Fractions and SNe Ia
• Can residuals of the Solar system foreground explain low multipole anomalies of the CMB ?
• Phenomenological Aspects of Heterotic Orbifold Models at One Loop
• Brane-Bulk energy exchange and agegraphic dark energy
• Probing large-scale magnetism with the Cosmic Microwave Background
• Analytical model of dark energy stars
• Second-order gravitational effects of local inhomogeneities on CMB anisotropies in nonzero-Lambda flat cosmological models
• Can gamma-ray bursts constrain quintessence?
• Probing the Impact of WIMP Dark Matter on Universal Relations, GW170817 Posterior and Radial Oscillations
• Making waves on CMB power spectrum and inflaton dynamics
• Sourced Friedmann equations with holographic energy density
• SILC: a new Planck Internal Linear Combination CMB temperature map using directional wavelets
• Gravitational Dust Collapse in $f(R)$ Gravity
• Wormhole solutions with a complex ghost scalar field and their instability
• Semiclassics of the Chaotic Quantum-Classical Transition
• Long term X-Ray Observations of Seyfert 1 Galaxy Ark 120: On the origin of soft-excess
• Transient Crossing of Phantom divide line $w_{\Lambda }=-1$ under Gauss-Bonnet interaction
• The Formation and Evolution of the First Massive Black Holes
• Study of the charged super-Chandrasekhar limiting mass white dwarfs in the $f(R,\mathcal{T})$ gravity
• Matter-Antimatter Asymmetry in the Large Hadron Collider
• Interacting $F(R,T)$ gravity with modified Chaplygin gas
• Heteroclinic orbit and tracking attractor in cosmological model with a double exponential potential
• Space-time correlations in inflationary spectra, a wave packet analysis
• Corrected holographic dark energy with power-law entropy and Hubble Horizon cut-off in FRW Universe
• Cosmological evolution of cosmic strings with time-dependent tension
• An oscillating Universe from the linearized R^{2} theory of gravity
• Traversable holographic dark energy wormholes constrained by astronomical observations
• Is the cold spot responsible for the CMB North-South asymmetry?
• Physics Opportunities with a TeV Linear Collider
• Group theoretical interpretation of the modified gravity in de Sitter space
• Observations of the Cosmic Microwave Background and Galactic Foregrounds at 12-17 GHz with the COSMOSOMAS Experiment
• Dynamics of an Anisotropic Universe in $f(R,T)$ Theory
• Cosmic Polarization Rotation, Cosmological Models, and the Detectability of Primordial Gravitational Waves
• Gravitational Baryogenesis in Running Vacuum models
• A framework for testing isotropy with the cosmic microwave background
• The large-scale bias of the hard X-ray background
• A directional continuous wavelet transform on the sphere
• The Principle of Relativity and Special Relativity Triple
• Attractor Solution in Coupled Yang-Mills Field Dark Energy Models
• Testing homogeneity with galaxy number counts : light-cone metric and general low-redshift expansion for a central observer in a matter dominated isotropic universe without cosmological constant
• Dark matter and Colliders searches in the MSSM
• CMB statistical anisotropy, multipole vectors and the influence of the dipole
• WMAP-Compliant Benchmark Surfaces for MSSM Higgs Bosons
• The Draco dwarf galaxy in the near-infrared
• The One-dimensional Fourier Representation and Large Angular Scale Foreground Contamination in the 3-year Wilkinson Microwave Anisotropy Probe data
• Bayesian analysis of bulk viscous matter dominated universe
• Hints of star fomation at z>6: the chemical abundances of the DLA system in the QSO BRI 1202-0725 (z_abs = 4.383)
• The Seeds of Cosmic structure as a door to New Physics
• Radiation in the process of the formation of voids
• A stable flat universe with variable Cosmological constant in f(R,T) Gravity
• Geometrical Origin of the Cosmological Constant
• Magnetic field in holographic superconductor with dark matter sector
• Bianchi type-I Dust Filled Accelerating Brans- Dicke Cosmology
• Friedmann Equation for Brans Dicke Cosmology
• Schrödinger-Wheeler-DeWitt equation in chaplygin gas FRW cosmological model
• Fluctuating annihilation cross sections and the generation of density perturbations
• Non-Gaussianity due to Possible Residual Foreground Signals in WMAP 1st-year Data Using Spherical Wavelet Approaches
• Antenna Instrumental Polarization and its Effects on E- and B-Modes for CMBP Observations
• Cosmological implications of interacting polytropic gas dark energy model in non-flat universe
• CP Asymmetries of $B\to \varphi K$ and $B\to {\eta }^{(\prime )}K$ Decays Using a Global Fit in QCD Factorization
• The imprint of cosmological hydrogen recombination lines on the power spectrum of the CMB
• CMB Anisotropies Reveal Quantized Gravity
• The field surrounding NGC 7603: cosmological or non-cosmological redshifts?
• Potential--density pairs for spherical galaxies and bulges: the influence of scalar fields
• Cosmography of interacting generalized QCD ghost dark energy
• Surface vacuum energy and stresses for a brane in de Sitter spacetime
• Tomography from the Next Generation of Cosmic Shear Experiments for Viable f(R) Models
• Bianchi type II models in the presence of perfect fluid and anisotropic dark energy
• Generalised scalar-tensor theory and the cosmic acceleration
• Long-term monitoring of Ark 120 with Swift
• Ellipticity in Cosmic Microwave Background as a Tracer of Large-Scale Universe
• Twenty Years of SUGRA
• Sunyaev-Zeldovich effect in WMAP and its effect on cosmological parameters
• Neutrinoless double beta decay and neutrino mass hierarchies
• Big-bang nucleosynthesis in Brans-Dicke cosmology with a varying $\Lambda$ term related to WMAP
• The polyhedral nature of LINERs: An XMM-Newton view of LINERs in radio galaxies
• Estimating N-Point Correlation Functions from Pixelized Sky Maps
• On the bispectrum of COBE and WMAP
• Auto and cross correlation of phases of the whole-sky CMB and foreground maps from the 1-year WMAP data
• Tessellated Mapping of Cosmic Background Radiation Correlations and Source Distributions
• Dynamical System Analysis for a phantom model
• Evidence for horizon-scale power from CMB polarization
• The simplest parametrization of equation of state parameter in the scalar field Universe
• Improved calculation of relic gravitational waves
• The Amplitude of Dark Energy Perturbations
• 4U 1344-60: a bright intermediate Seyfert galaxy at z=0.012 with a relativistic Fe Kalpha emission line
• Naturalness in Cosmological Initial Conditions
• Chaplygin gas may prevent big trip
• The nature of a broad line radio galaxy: Simultaneous RXTE and Chandra HETG observations of 3C 382
• Sneutrino condensate as a candidate for the hot big bang cosmology
• CMB Polarization due to Scattering in Clusters
• The effect of asymmetric beams in the Wilkinson Microwave Anisotropy Probe experiment
• On Cosmological Implications of Gravitational Trace Anomaly
• A comparison between direct and indirect dark matter search
• Building the full PMNS Matrix from six independent Majorana-type phases
• On dark matter search after DAMA with Ge-73
• Phantom Instability of Viscous Dark Energy in Anisotropic Space-Time
• Cosmological test of the Yilmaz theory of gravity
• Planar distribution of the galaxies in the Local Group: a statistical and dynamical analysis
• Predicting the CMB power spectrum for binary polyhedral spaces
• Observational Constraints on a Variable Dark Energy Model
• A Beginner's Guide to the Theory of CMB Temperature and Polarization Power Spectra in the Line-of-Sight Formalism
• A study of phantom scalar field cosmology using Lie and Noether symmetries
• A New Type of Dark Energy Model
• Holographic interacting dark energy in the braneworld cosmology
• Dynamics of Quintessential Inflation
• On the Amount of Gravitational Waves from Inflation
• Strongly lensed type Ia supernovae as a precise late-universe probe of measuring the Hubble constant and cosmic curvature
• Combined LHC/ILC analysis of a SUSY scenario with heavy sfermions
• Cosmic Evolution in Self-Interacting Brans-Dicke Cosmology
• Standard Cosmological Evolution in f(R) Model to Kaluza Klein Cosmology
• Eigenmode Analysis of Galaxy Distributions in Redshift Space
• COBE-DMR-Normalized Dark Energy Cosmogony
• Stochastic gravitoelectromagnetic inflation
• Grand Unified Inflation Confronts WMAP
• Stability of a Class of Non-Static Axial Self-Gravitating Systems in $f(R)$ Gravity
• Effect of the Metallicity on the X-ray Emission from the Warm-Hot Intergalactic Medium
• Noether Symmetry Analysis of Anisotropic Universe in Modified Gravity
• Lepton asymmetry in the primordial gravitational wave spectrum
• Test of conformal gravity with astrophysical observations
• Black-Body Radiation Of Noncommutative Gauge Fields
• Forecast for the Next Eon: Applied Cosmology and the Long-Term Fate of Intelligent Beings
• Transverse Wave Propagation in Relativistic Two-fluid Plasmas around Schwarzschild-de Sitter Black Hole
• Supergravity Minimal Inflation and its Spectral Index Revisited
• Calibration of Transition-edge Sensor (TES) Bolometer Arrays with Application to CLASS
• Multipole invariants and non-Gaussianity
• Leptogenesis by curvature coupling of heavy neutrinos
• Holographic Dark Energy Model and Scalar-Tensor Theories
• Imperfect fluid cosmological model in modified gravity
• New constraint on the cosmological background of relativistic particles
• Cosmological constraints on polytropic gas model
• Foreground analysis from the 1-year Wilkinson Microwave Anisotropy Probe (WMAP) data
• CMB in a box: causal structure and the Fourier-Bessel expansion
• On the impact of large angle CMB polarization data on cosmological parameters
• The Cosmological Unimportance of Low Surface Brightness Galaxies
• Dark Energy: The Observational Challenge
• Cosmological parameters in the noncommutative inflation
• Phase-space of flat Friedmann-Robertson-Walker models with both a scalar field coupled to matter and radiation
• Squeezing MOND into a Cosmological Scenario
• The end of the Dark Ages in MOND
• Testing cosmological models and understanding cosmological parameter determinations with metaparameters
• Casimir energy-momentum tensor for the Robin Surfaces in de Sitter Spacetime
• Latest data constraint of some parameterized dark energy models
• Dominant Multipoles in WMAP5 Mosaic Data Correlation Maps
• Stability of Accelerated Expansion in Nonlinear Electrodynamics
• The Complementarity of Redshift-space Distortions and the Integrated Sachs-Wolfe Effect: A 3D Spherical Analysis
• Dark energy stars: Stable configurations
• Viscous universe with cosmological constant
• Phase space analysis of the bouncing universe with stringy effects
• Extragalactic Point Source Search in WMAP 61 and 94 GHz Data
• Prospects for Dark Energy Evolution: a Frequentist Multi-Probe Approach
• FRW model with Two -- fluid Source in fractal cosmology
• Modeling the large-scale power deficit with smooth and discontinuous primordial spectra
• Open inflationary universes in a brane world cosmology
• Perturbations for transient acceleration
• The Confining Heterotic Brane Gas: A Non-Inflationary Solution to the Entropy and Horizon Problems of Standard Cosmology
• A brief review on cosmological analysis of galaxy surveys with multiple tracers
• Gamma-ray detection from neutralino annihilation in non--universal SUGRA scenarios
• Phase Space Analysis and Thermodynamics of Interacting Umami Chaplygin gas in FRW Universe
• Foreground contributions to the Cosmic Microwave Background
• Cosmological models with squared trace in modified gravity
• Clustering of SZ clusters on a past light-cone: acoustic oscillations and constraints on dark energy
• Gravitational collapse due to dark matter and dark energy in the brane world scenario
• Probing the largest scale structure in the universe with polarization map of galaxy clusters
• Gauss-Bonnet braneworld cosmological effect on relic density of dark matter
• Mimetic Attractors
• Some Plane Symmetric Inhomogeneous Cosmological Models in the Scalar-Tensor Theory of Gravitation
• Constraints On The Topology Of The Universe From The WMAP First-Year Sky Maps
• Reconstructing Dark Matter Density with e^+e^- Linear Collider in Focus-Point Supersymmetry
• CMB component separation in the pixel domain
• Scalar statistics on the sphere: application to the CMB
• On the age and mass function of the globular cluster M4: a different interpretation of recent deep HST observations
• Probing Baryogenesis in $f(Q)$ gravity
• Cosmic microwave background power spectrum estimation with the destriping technique
• Cosmoglobe DR1 results. I. Improved Wilkinson Microwave Anisotropy Probe maps through Bayesian end-to-end analysis
• On the Dirac field in the Palatini form of 1/R gravity
• The Discovery of Extended Thermal X-ray Emission from PKS 2152-699: Evidence for a `Jet-cloud' Interaction
• Power-law entropy-corrected HDE and NADE in Brans-Dicke cosmology
• An Inverse $f(R)$ Gravitation for Cosmic Speed up, and Dark Energy Equivalent
• Charge Conjugation Invariance of the Vacuum and the Cosmological Constant Problem
• Detectability of Cosmic Topology in Flat Universes
• A polarized synchrotron template for CMBP experiments after WMAP data
• Inflationary attractor in Gauss-Bonnet brane cosmology
• From radio-quiet to radio-silent: low luminosity Seyfert radio cores
• Probing Nuclear and Circumnuclear Properties of NGC 6300 using X-ray Observations
• Kaluza-Klein Type Robertson Walker Cosmological Model With Dynamical Cosmological Term $\Lambda$
• Constraints on non-resonant photon-axion conversion from the Planck satellite data
• Constraining the topology of the Universe using the polarised CMB maps
• General quadrupolar statistical anisotropy: Planck limits
• QCD modified ghost scalar field dark energy models
• Statistical Characterization of Temperature Patterns in Anisotropic Cosmologies
• Searching for primordial non-Gaussianity in Planck CMB maps using a combined estimator
• Growth of perturbations in dark energy parametrization scenarios
• From the production of primordial perturbations to the end of inflation
• Template fitting of WMAP 7-year data: anomalous dust or flattening synchrotron emission?
• Large-scale anomalies of the CMB in the curvaton scenario
• Universe opacity and CMB
• Supersymmetric extra U(1) models with a singlino dominated LSP
• From model dynamics to oscillating dark energy parameterisation
• From BeyondPlanck to Cosmoglobe: Preliminary $WMAP$ $Q$-band analysis
• Observing other universe through ringholes and Klein-bottle holes
• B polarization of cosmic background radiation from second-order scattering sources
• Least-action perihelion precession
• Sneutrino brane inflation and leptogenesis
• Gravitational Lensing by Dark Matter Caustics
• Dark energy and dark matter from an inhomogeneous dilaton
• Integrated field spectroscopy of E+A (post-starburst) galaxies with the Kyoto3DII
• The effect of reionization on the CMB-density correlation
• Trade-off between angular resolution and straylight contamination in CMB anisotropy experiments. II. Straylight evaluation
• Mapping the large-angle deviation from Gaussianity in simulated CMB maps
• Local properties of WMAP Cold Spot
• Interacting entropy-corrected holographic dark energy with apparent horizon as an infrared cutoff
• Bianchi Type-I Universe Models with Nonlinear Viscosity
• Thermal and non-thermal emission in the Cygnus X region
• CMB polarization as a probe of the anomalous nature of the Cold Spot
• Gravitational, shear and matter waves in Kantowski-Sachs cosmologies
• The Hot and Cold Spots in Five-Year WMAP Data
• Scale of Homogeneity of the Universe from WMAP
• Gravity and Mirror Gravity in Plebanski Formulation
• Cosmic polarimetry in magnetoactive plasmas
• LRS Bianchi type-I bulk viscous cosmological models in $f(R,T)$ gravity
• Dark Energy Models With Variable Equation Of State Parameter
• [OIII] profile substructure in radio-quiet quasars
• Measuring the Mach number of the Universe via the Sunyaev-Zeldovich effect
• Revised estimates of CMB $B$-mode polarization induced by patchy reionization
• The Integrated Sachs-Wolfe effect as a probe of non-standard cosmological evolution
• Peculiarities of phases of the WMAP quadrupole
• Dark Energy and Neutrino CPT Violation
• Constant-Roll Inflation in modified $f(R,\varphi )$ gravity model using Palatini Formalism
• Bianchi VII_h models and the cold spot texture
• Molecular fluorine chemistry in the early Universe
• A Note on Noncommutative Brane Inflation
• The Angular Power Spectrum of the First-Year WMAP Data Reanalysed
• Strong lensing by cluster-sized haloes in dark-energy cosmologies
• Sunyaev-Zel'dovich Cluster Survey Simulations for Planck
• Dark Matter in the Simplest Little Higgs Model
• The variance of the CMB temperature gradient: a new signature of a multiply connected Universe
• On Bianchi type III Cosmological Model with Quadratic EoS in Lyra Geometry
• Slice Energy in Higher Order Gravity Theories and Conformal Transformations
• Bounds on the Neutrino Mixing Angles and CP Phase for an SO(10) Model with Lopsided Mass Matrices
• Constraints on Supersymmetry from Relic Density compared with future Higgs Searches at the LHC
• How heavy can the Fermions in Split Susy be? A study on Gravitino and Extradimensional LSP
• Rigidity of cosmic acceleration in a class of k-essence cosmologies
• On the dipole straylight contamination in spinning space missions dedicated to CMB anisotropy
• Tachyonic open inflationary universes
• Non-Gaussianity in the Very Small Array CMB maps with Smooth-Goodness-of-fit tests
• Information on the inflaton field from the spectrum of relic gravitational waves
• Cosmic microwave background polarization analysis
• Big Bang Nucleosynthesis with an Evolving Radion in the Brane World Scenario
• Electromagnetic dark energy
• Statefinder parameters for quantum effective Yang-Mills condensate dark energy model
• Thermodynamical properties of dark energy with the equation of state
• Precision Primordial ${}^4$He Measurement with CMB Experiments
• LISA and LISA PathFinder, the endeavour to detect low frequency GWs
• The generalized second law for the interacting new agegraphic dark energy in a non-flat FRW universe enclosed by the apparent horizon
• Cosmological Solutions with Torsion in a Model of de Sitter Gauge Theory of Gravity
• Detection of blueshifted emission and absorption and a relativistic Iron line in the X-ray spectrum of ESO 323-G077
• Natural braneworld inflation and baryogenesis
• Non-Gaussian Foreground Residuals of the WMAP First Year Maps
• Direct Search for Dark Matter - Striking the Balance - and the Future
• Correlations from Galactic foregrounds in the 1-year Wilkinson Microwave Anisotropy Probe WMAP data
• Cosmological constant and gravitational theory on D-brane
• Embedding of FRW Cosmology in DGP Scenario with a Non-Minimally Coupled Scalar Field on the Brane
• FLRW accelerating universe with interactive dark energy
• Detecting Intracluster Gas Motion in Galaxy Clusters: Mock Astro-E2 Observations
• Enhanced reheating via Bose condensates
• On the effect of cyclotron emission on the spectral distortions of the cosmic microwave background
• De-Sitter nonlinear sigma model and accelerating universe
• De Sitter Thermodynamics from Diamonds's Temperature
• High-impedence NbSi TES sensors for studying the cosmic microwave background radiation
• Interacting agegraphic quintessence dark energy in non-flat universe
• Asymfast, a method for convolving maps with asymmetric main beams
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• On the driver of relativistic effects strength in Seyfert galaxies
• Standard siren cosmology in the era of the 2.5-generation ground-based gravitational wave detectors: bright and dark sirens of LIGO Voyager and NEMO
• The Higgs intense--coupling regime in constrained SUSY models and its astrophysical implications
• Implementation of a Fourier Matched Filter in CMB Analyses. Application to ISW Studies
• Dark Energy Models and Laws of Thermodynamics in Bianchi I Model
• Indirect Signals from Dark Matter in Split Supersymmetry
• Is Thick Brane Model Consistent with the Recent Observations?
• The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey
• Cosmological Constraints on the DGP braneworld model with Gamma-ray bursts
• Logarithmic entropy corrected holographic dark energy with $F(R,T)$ gravity
• Introduction to neutrino cosmology
• Electroweak Baryogenesis from Late Neutrino Masses
• Non-thermal leptogenesis via direct inflaton decay without SU(2)(L) triplets
• CMB Observations with a Compact Heterogeneous 150 GHz Interferometer in Chile
• Cosmic Acceleration and Brans-Dicke Theory
• The Reionization History and Early Metal Enrichment inferred from the Gamma-Ray Burst Rate
• 7 mm continuum observations of ultra compact HII regions
• Leptogenesis as the source of gravitino dark matter and density perturbations
• The local dust foregrounds in the microwave sky: I. Thermal emission spectra
• Recombination Induced Softening and Reheating of the Cosmic Plasma
• $f(\mathcal{G},\text{T})$ Gravity Bouncing Universe with Cosmological Parameters
• Potential-density pairs for axisymmetric galaxies: the influence of scalar fields
• Data compression on the sphere
• Real space tests of the statistical isotropy and Gaussianity of the WMAP CMB data
• Likelihood, Fisher information, and systematics of cosmic microwave background experiments
• Ellipticity analysis of the BOOMERanG CMB maps
• Evolution of the Cluster Correlation Function
• Observational Constraints on Undulant Cosmologies
• Probing violation of the Copernican principle via the integrated Sachs-Wolfe effect
• A minimal set of invariants as a systematic approach to higher order gravity models
• Noether Symmetries of a Modified Model in Teleparallel Gravity and a New Approach for Exact Solutions
• Chaplygin inflation in loop quantum cosmology
• Dynamics of Axial Symmetric System in Self-Interacting Brans-Dicke Gravity
• An expanding 4D universe in a 5D Kaluza-Klein cosmology with higher dimensional matter
• Non-thermal leptogenesis and baryon asymmetry in different neutrino mass models
• On the suspected timing-offset-induced calibration error in the Wilkinson microwave anisotropy probe time-ordered data
• Curvature corrections in DGP brane cosmology
• On the Rees-Sciama effect: maps and statistics
• A New Class of Bianchi Type-I Cosmological Models in Scalar-Tensor Theory of Gravitation and Late Time Acceleration
• The WSRT Virgo HI filament survey I; Total Power Data
• Measuring kinematic anisotropies with pulsar timing arrays
• A Classical Treatment of Island Cosmology
• Weighing neutrinos in the presence of a running primordial spectral index
• Leptogenesis, neutrino masses and gauge unification
• Tomography of the Reionization Epoch with Multifrequency CMB Observations
• Cosmological Tests of $f(R,G,T)$ Dark Energy Model in FRW Universe
• String Theory, Space-Time Non-Commutativity and Structure Formation
• Partial wave treatment of Supersymmetric Dark Matter in the presence of CP - violation
• Limits on the Polarization of the Cosmic Microwave Background Radiation at Multipoles up to l~2000
• The final verdict by XMM-Newton: the X-ray obscured Seyfert galaxy NGC5506 has a broad Fe K-alpha line
• An FLRW interacting dark energy model of the Universe
• Long-Term X-Ray spectral variability of the radio-loud NLS1 galaxy PKS 0558-504
• Correlations Between the WMAP and MAXIMA Cosmic Microwave Background Anisotropy Maps
• Direct and Indirect Detection of Dark Matter in Heterotic Orbifold Models
• Observational Scan Induced Artificial CMB Anisotropy
• Electrostatic and Magnetostatic Solutions in a Lorentz-Violating Electrodynamics Model
• Beyond the Standard Model
• Production of Long-Lived Sleptons at LHC
• Dark Energy Nature in Logarithmic $f(R,T)$ Cosmology
• The XMM-Newton spectrum of the high-z optically-obscured QSO RX J1343.4+0001: a classic radio quiet QSO
• Ricci-Gauss-Bonnet holographic dark energy in Chern-Simons modified gravity: A flat FLRW quintessence-dominated universe
• Why do we Still Believe in Newton's Law ? Facts, Myths and Methods in Gravitational Physics
• Generalized Self-similar Scalar-Tensor Theories
• A stable flat entropy-corrected FRW universe
• Charged Higgs Bosons in the MSSM at CMS: Discovery Reach and Parameter Dependence
• Vacuum fluctuations of the supersymmetric field in curved background
• Mass spectrum of primordial black holes from inflationary perturbation in the Randall-Sundrum braneworld: a limit on blue spectra
• Does Transparent Hidden Matter Generate Optical Scintillation?
• Non-minimal Split Supersymmetry
• Can Strong Gravitational Lensing Constrain Dark Energy?
• Data analysis methods for the cosmic microwave background
• The X-ray variability history of Markarian 3
• CMB Polarization and Temperature Power Spectra Estimation using Linear Combination of WMAP 5-year Maps
• f(R) Gravity in an Ellipsoidal Universe
• Hemispherical Power Asymmetry in intensity and polarization for Planck PR4 data
• Higgsino dark matter in partly supersymmetric models
• Testing CMB Anomalies in E-mode Polarization with Current and Future Data
• Can brane dark energy model be probed observationally by distant supernovae?
• Low Scale Seesaw, Electron EDM and Leptogenesis in a Model with Spontaneous CP Violation
• Configurational Entropy and braneworlds in f(T,B) gravity
• Efficient ILC analysis on polarization maps after EB leakage correction
• Scalar field potentials for cosmology
• Dark Matter Constraints on Gaugino/Higgsino Masses in Split Supersymmetry and Their Implications at Colliders
• A flat FRW model with dynamical $\Lambda$ as function of matter and geometry
• New physics from ultrahigh energy cosmic rays
• FRW dark energy cosmological model with hybrid expansion law
• Degeneracy of consistency equations in braneworld inflation
• Extra-Dimensions and Dark Matter
• Angular power spectrum of CMB anisotropy from WMAP
• Expected constraints on the Galactic magnetic field using PLANCK data
• On the viability of Planck scale cosmology with quartessence
• The Angular-Diameter-Distance-Maximum and Its Redshift as Constraints on $\Lambda \ne 0$ FLRW Models
• Nontrivial Geometries: Bounds on the Curvature of the Universe
• Noether symmetry in the Nash theory of gravity
• Correlated Hybrid Fluctuations from Inflation with Thermal Dissipation
• Modular thermal inflation without slow-roll approximation
• The Unified Equation of State for Dark Matter and Dark Energy
• X-ray Absorption Toward Abell 2029 due to a Foreground Spiral
• NGC 6240 Supermassive Black Hole Binary dynamical evolution based on Chandra data
• Cosmological Parameter Estimation Using Current and Future Observations of Strong Gravitational Lensing
• Cosmological Constant in a Model with Superstring-Inspired E_6 Unification and Shadow Theta-Particles
• Small scale contributions to CMB: A coherent analysis
• Whether Lyra's Manifold Itself is a Hidden Source of Dark Energy
• An analytic approach to perturbations from an initially anisotropic universe
• On the anomalous red giant branch of the globular cluster Omega Cen
• Scaling Dark Energy
• GRB Sky Distribution Puzzles
• Induced CMB quadrupole from pointing offsets
• Effect of Foregrounds on the CMBR Multipole Alignment
• Large Scale Traces of Solar System Cold Dust on CMB Anisotropies
• Molecular hydrogen in the cosmic recombination epoch
• Exploring Plane Symmetric Solutions in $f(R)$ Gravity
• On the absence of gravitational lensing of the cosmic microwave background
• Thermodynamics of Modified Chaplygin Gas and Tachyonic Field
• First Results of the 74 MHz VLA-Pie Town Link. Hercules A at Low Frequencies
• Holographic dark energy with time varying $c^2$ parameter
• An H-alpha nuclear spiral structure in the E0 active galaxy Arp102B
• Non-commutative Power-law Inflation: Mode Equation and Spectra Index
• Inflating p-branes
• Power-law entropy corrected new holographic scalar field models of dark energy with modified IR-cutoff
• Inverse-Scattering Theory and the Density Perturbations from Inflation
• Quantum cosmic models and thermodynamics
• Cosmological constant in SUGRA models with Planck scale SUSY breaking and degenerate vacua
• An indirect dark matter search with diffuse gamma rays from the Galactic Centre with the Alpha Magnetic Spectrometer
• Interacting generalized ghost dark energy in non-flat universe
• Dark Energy Cosmology with the Alternative Cosmic Microwave Background Data
• Dodecahedral topology fails to explain quadrupole-octupole alignment
• Intracluster Entropy from Joint X-ray and Sunyaev-Zel'dovich Observations
• Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys
• The impact of dipole straylight contamination on the alignment of low multipoles of CMB anisotropies
• Anisotropic Galactic Outflows and Enrichment of the Intergalactic Medium. II. Numerical Simulations
• Dynamical quintessence fields Press-Schechter mass function: detectability and effect on dark haloes
• On the suspected timing error in WMAP map-making
• Issues in the Philosophy of Cosmology
• Thermodynamics of Shearing Massless Scalar Field Spacetimes is Inconsistent With the Weyl Curvature Hypothesis
• Simplified Quartessence Cosmology
• Observation constraints on scalar field cosmological model in Anisotropic universe
• Probing galaxy density profiles with future supernova surveys
• Cosmological dynamics of scalar fields with O(N) symmetry
• Signals of sneutrino-antisneutrino mixing in an $e^{-}\gamma$ collider in anomaly-mediated supersymmetry breaking
• Millimeter observations of Planetary Nebulae: a contribution to the Planck pre-launch catalogue
• Sneutrino inflation in Gauss-Bonnet brane-world cosmology, the gravitino problem and leptogenesis
• From heaviness to lightness during inflation
• Nonsingular density profiles of dark matter halos and Strong gravitational lensing
• The N-Tachyon Assisted Inflation
• Fractal Structure of Isothermal Lines and Loops on the Cosmic Microwave Background
• H_2 Line Emission Associated with the Formation of the First Stars
• Higher-order generalized uncertainty principle applied to gravitational baryogenesis
• Light mass galileon and late time acceleration of the Universe
• Observational constraints on the braneworld model with brane-bulk energy exchange
• Analytic Spectra of CMB Anisotropies and Polarization Generated by Scalar Perturbations in Synchronous Gauge
• Relativistic Effects of our Galaxy's Motion on Circles-in-the-sky
• A Chandra Study of the Core of the Nearby Cluster Abell 576
• Sneutrino Inflation
• A Modified Generalized Chaplygin Gas as the Unified Dark Matter-Dark Energy Revisited
• $\delta T/T$ and Neutrino Masses in SU(5)
• (A)symmetric Tachyon Rolling in de Sitter Spacetime: A universe devoid of Planck density
• Magnesium abundances in mildly metal-poor stars from different indicators
• Entropy and statefinder diagnosis in chameleon cosmology
• Universe Bounded By Event Horizon: A Non equilibrium Thermodynamic Prescription
• Bianchi type-VI anisotropic dark energy model with varying EoS parameter
• Anisotropic evolution of 5D Friedmann-Robertson-Walker spacetime
• Implications of cosmic strings with time-varying tension on CMB and large scale structure
• XMM-Newton view of galaxy pairs: activation of quiescent black holes?
• Quintessence and the Curvature of the Universe after WMAP
• Scale Invariant Spectrum from Variable Speed of Light Metric in a Bimetric Gravity Theory
• Foreground removal from CMB temperature maps using an MLP neural network
• Consistency of Equations in the Second-order Gauge-invariant Cosmological Perturbation Theory
• Unravelling the Dark Matter - Dark Energy Paradigm
• Observational constrained Weyl type $f(Q,T)$ gravity cosmological model and the dynamical system analysis
• Weyl Anomaly and Initial Singularity Crossing
• Asymptotic behavior of Cardassian cosmologies with exponential potentials
• Charged gravastar model in $f(T)$ gravity admitting conformal motion
• Interacting new agegraphic Phantom model of dark energy in non-flat universe
• Some high-frequency gravitational waves related to exact radiative spacetimes
• Gravitational Baryogenesis in Ho$\check{r}$ava-Lifshitz gravity
• Assessment of the Systematic Uncertainties in the Cosmological Analysis of the SDSS Supernovae Photometric Sample
• Assisted Inflation from Geometric Tachyon
• Frequentist comparison of CMB local extrema statistics in the five-year WMAP data with two anisotropic cosmological models
• Dark Matter in Fractional Gravity I: Astrophysical Tests on Galactic Scales
• Cosmological determination to the values of the prefactors in the logarithmic corrected entropy-area relation
• Gravitation, electromagnetism and the cosmological constant in purely affine gravity
• Cosmological constraints on a dark matter -- dark energy interaction
• Non-flat universe and interacting dark energy model
• The spectral index of polarized diffuse Galactic emission between 30 and 44 GHz
• On the Effects due to a Decaying Cosmological Fluctuation
• Classification of Cosmic Scale Factor via Noether Gauge Symmetries
• Site Evaluation and RFI spectrum measurements in Portugal at the frequency range 0.408-10 GHz for a GEM polarized galactic radio emission experiment
• Spatially Resolved Spectroscopy of Passive Spiral Galaxies
• Approximate Consistency Condition from Running Spectral Index in Slow-Roll Inflationary Models
• Perturbations of the Yang-Mills field in the universe
• Polarized Spots in Anisotropic Open Universes
• Is flat rotation curve a sign of cosmic expansion?
• Hamiltonian perturbation theory in f(R) gravity
• Observational Constraints on Axions as Quintessence in String Theory
• Testing for spectral index variations in polarised CMB foregrounds
• Evidence for Inverted Spectrum 20 GHz Emission in the Galactic Plane
• Scale dependence of the primordial spectrum from combining the three-year WMAP, Galaxy Clustering, Supernovae, and Lyman-alpha forests
• Real space tomography of the primordial Universe with cluster polarization
• F(R) cosmology via Noether symmetry and lambda-Chaplygin Gas like model
• A Quantum Cosmology: No Dark Matter, Dark Energy nor Accelerating Universe
• Dilaton and Moduli Fields in D-term inflation
• Observations of Free-Free and Anomalous Microwave Emission from LDN 1622 with the 100 m Green Bank Telescope
• Dynamics of Domain Walls for Split and Runaway Potentials
• Baryogenesis and the New Cosmology
• Measuring Dark Matter Flows in Merging Clusters of Galaxies
• Phenomenology of a 5D Orbifold $SU(3{)}_W$ Unification model
• A spherical scalar-tensor galaxy model
• Modelling Tachyon Cosmology with Non-Minimal Derivative Coupling to Gravity
• Modeling and Analyzing Stability of Hybrid Stars within $f(Q)$ Gravity
• Varying Alpha Monopoles
• Fast calculation of the Fisher matrix for cosmic microwave background experiments
• Post-inflation increase of the cosmological tensor-to-scalar perturbation ratio
• Sunyaev-Zel'dovich Signal from Quasar Hosts: Implications for Detection of Quasar Feedback
• Chaplygin Gas Hořava-Lifshitz Quantum Cosmology
• Cosmological models of generalized ghost pilgrim dark energy (GGPDE) in the gravitation theory of Saez-Ballester
• Quantum cosmology for non-minimally coupled scalar field in FLRW space-time: A symmetry analysis
• Cosmic Strings and the Origin of Globular Clusters
• Measured Cosmological Mass Density in the WHIM: the Solution to the 'Missing Baryons' Problem
• The current status of observational cosmology
• Gravitational Waves in Locally Rotationally Symmetric (LRS) Class II Cosmologies
• Correlation of supernova redshifts with temperature fluctuations of the Cosmic Microwave Background
• Density fluctuations in $\kappa$-deformed inflationary universe
• Dark matter candidate in an extended type III seesaw scenario
• Phase analysis of the cosmic microwave background from an incomplete sky coverage
• Blackbody radiation in κ-Minkowski spacetime
• Neutrino Dark Energy With More Than One Neutrino Species
• Non-minimally coupled quintessence DE model with a cubic galileon term --A Dynamical System Analysis
• Some doubts on the validity of the foreground Galactic contribution subtraction from microwave anisotropies
• Foreground removal from WMAP 5yr temperature maps using an MLP neural network
• Neutron Diffusion and Nucleosynthesis in an Inhomogeneous Big Bang Model
• Halting eternal acceleration with an effective negative cosmological constant
• Deep redshift topological lensing: strategies for the T^3 candidate
• The size of the Universe according to the Poincare dodecahedral space hypothesis
• Cosmology With Axionic-quintessence Coupled with Dark Matter
• Cosmological simulations using a static scalar-tensor theory
• Discrete Spectrum of Inflationary Fluctuations
• Irreversible thermodynamics of dark energy on entropy-corrected apparent horizon
• Revisit of constraints on dark energy with Hubble parameter measurements including future redshift drift observations
• Polytropic gas scalar field models of dark energy
• Weak gravitational lensing by compact objects in fourth order gravity
• Symmetry of the CMB sky as a new test of its statistical isotropy. Non Cosmological Octupole?
• Flavour Structure of R-violating Neutralino Decays at the LHC
• Chance and Chandra (and repulsive dark matter)
• The universe dynamics in the tachyon cosmology with non-minimal coupling to matter
• MiXDM: Cosmic Ray Signals from Multiple States of Dark Matter
• Energy Constraints and $F(T,T_G)$ Cosmology
• Fractal Bubble Cosmology: A concordant cosmological model?
• Brane inflation revisited after WMAP five-year results
• Anisotropy effects on Baryogenesis in $f(R)$-Theories of Gravity
• Late-time acceleration with steep exponential potentials
• Large Lepton Mixings from Continuous Symmetries
• Thermodynamics in a Modified Gravity Involving Higher-Order Torsion Derivative Terms
• Testing the scale-dependent hemispherical asymmetry with the 21-cm power spectrum from the epoch of reionization
• New Horizons in Cosmology with Spectral Distortions of the Cosmic Microwave Background
• Effect of the length of inflation on angular TT and TE power spectra in power-law inflation
• Brane gas-driven bulk expansion as a precursor stage to brane inflation
• Massive Neutrinos in Cosmology
• The Revival of Cosmic Strings
• Biases to primordial non-Gaussianity measurements from CMB secondary anisotropies
• On the response of the Einstein Telescope to Doppler anisotropies
• Fractal FRW Model within Domain Wall
• Astrophysical Observations: Lensing and Eclipsing Einstein's Theories
• Effect of component separation on the temperature distribution of the CMB
• Synthesis of H-alpha absorption in old stellar systems: Formation of the cluster red sequence by "Downsizing"
• Observational Constraints on Varying Alpha in $\Lambda (\alpha )$CDM Cosmology
• Light Scalars and the Generation of Density Perturbations During Preheating or Inflaton Decay
• On the holographic dark energy in chameleon scalar-tensor cosmology
• Cosmological constraints on dark energy
• Towards a possible solution for the coincidence problem: f(G) gravity as background
• The interacting generalized Ricci dark energy model in non-flat universe
• Modified holographic Ricci dark energy coupled to interacting relativistic and non-relativistic dark matter in the nonflat universe
• Applications to cosmological models of a complex scalar field coupled to a U(1) vector gauge field
• Radiative Corrections to the Inflaton Potential as an Explanation of Suppressed Large Scale Power in Density Perturbations and the Cosmic Microwave Background
• Stability analysis in Modified Non-Local Gravity
• Discriminating neutrino mass models using Type II seesaw formula
• Cross-correlation between WMAP and 2MASS: non-Gaussianity induced by SZ effect
• Cosmic strings in Bekenstein-type models
• Numerical computation of Maass waveforms and an application to cosmology
• Models for Nonthermal Photon Spectra
• XMM-Newton view of the double-peaked Fe K-alpha complex in E1821+643
• Note on the Robustness of the Neutrino Mass Bounds from Cosmology
• A Cosmological Model with Dark Spinor Source
• Inflation on Fractional Branes: D--Brane Inflation as D--Term Inflation
• Evolution of magnetic component in Yang-Mills condensate dark energy models
• CMB power spectrum estimation with non-circular beam and incomplete sky coverage
• WMAP Data and Recent Developments in Supersymmetric Dark Matter
• Marginal distributions for cosmic variance limited CMB polarization data
• Gravitomagnetic effects in Kerr-de Sitter space-time
• Bayesian analysis of white noise levels in the 5-year WMAP data
• Is the misalignment of the Local Group velocity and the 2MASS Redshift Survey dipole typical in a LambdaCDM model?
• X-ray Clusters of Galaxies as Cosmological Tools
• Closed inflationary universe with tachyonic field
• Why CMB physics?
• Effective Search Templates for a Primordial Stochastic Gravitational Wave Background
• Trade-off between angular resolution and straylight contamination in CMB anisotropy experiments. I. Pattern simulations
• Mirror World with Broken Mirror Parity, E(6) Unification and Cosmology
• Consistency of a needlet spectral estimator on the sphere
• Domain structures in quantum graphity
• Cosmological Constraints on the Very Low Frequency Gravitational-Wave Background
• Temperature and Polarization Patterns in Anisotropic Cosmologies
• Baryon asymmetry from leptogenesis with four zero neutrino Yukawa textures
• Constraints from CMB in the intermediate Brans-Dicke inflation
• Inflation in anisotropic brane universe using tachyon field
• Prospects for the direct detection of neutralino dark matter in orbifold scenarios
• Leptogenesis in B-L gauged SUSY with MSSM Higgs sector
• Entropy-corrected new agegraphic dark energy in Horava-Lifshitz cosmology
• Revisiting the large-scale CMB anomalies: The impact of the SZ signal from the Local Universe
• X-ray and Sunyaev-Zeldovich properties of the WHIM
• The accelerated scaling attractor solution of the interacting agegraphic dark energy in Brans-Dicke theory
• Laboratory tests on dark energy
• Mixed fluid cosmological model in $f(R,T)$ gravity
• Quintessence models with an oscillating equation of state and their potentials
• Detection of Dipole Modulation in CMB Temperature Anisotropy Maps from WMAP and Planck using Artificial Intelligence
• Hadronic production and decays of Charginos and Neutralinos in Split Supersymmetry
• Spectral Indications of thermal Sunyaev-Zel'dovich Effect in Archeops and WMAP Data
• Seesaw Enhancement of Bi-large Mixing in Two-Zero Textures
• Scalar Field as Dark Energy Accelerating Expansion of the Universe
• Statistical properties of polarized CMB foreground maps
• Test of patch cosmology with WMAP
• Maxwell's Multipole Vectors and the CMB
• Testing the ABS method with the simulated Planck temperature maps
• A measurement of the Integrated Sachs-Wolfe Effect with the Rapid ASKAP Continuum Survey
• Isotropic non-Gaussian $g_{\mathrm{NL}}$-like toy models that reproduce the cosmic microwave background anomalies
• Pairwise kSZ signal extraction efficacy and optical depth estimation
• Multipole vectors of completely random microwave skies for $l\le 50$
• SUSY Resonances from UHE neutralinos in Neutrino Telescopes and in the Sky
• Can neutrino viscosity drive the late time cosmic acceleration?
• Non-Minimal Quintessence With Nearly Flat Potential
• Dynamics of Magnetized Bulk Viscous Strings in Brans-Dicke Gravity
• Forecasts of CMB lensing reconstruction of AliCPT-1 from the foreground cleaned polarization data
• Influence of Planck foreground masks in the large angular scale quadrant CMB asymmetry
• CMB maps lensed by cosmological structures: Simulations and statistical analysis
• Cross-Correlation analysis of WMAP and EGRET in Wavelet Space
• Gravitino dark matter from gluino late decay in split supersymmetry
• X-Ray Spectral Parameters for a Sample of 95 Active Galactic Nuclei
• Probing Particle Physics from Top Down with Cosmic Strings
• Sunyaev-Zel'dovich effect in the Virgo cluster from WMAP and ROSAT data
• Viscous Dark Energy and Phantom Field in An Anisotropic Universe
• Observational constraints and stability in viscous $f(T,\mathcal{T})$ gravity
• On the Einstein-Cartan cosmology vs. Planck data
• Early and Late-time Cosmic Acceleration in Non-minimal Yang-Mills-$f(G)$ Gravity
• Symmetries of CMB Temperature Correlation at Large Angular Separations
• Gauss-Bonnet braneworld and WMAP three year results
• Statistical physics for cosmic structures
• Light Propagation in Inhomogeneous Universes. V. Gravitational Lensing of Distant Supernovae
• Foreground removal with ILC methods for AliCPT-1
• Full-sky correlation functions for CMB experiments with asymmetric window functions
• Model of the polarized foreground diffuse Galactic emissions from 33 to 353 GHz
• Non-adiabatic perturbations in Ricci dark energy model
• Direct measurement of the angular power spectrum of cosmic microwave background temperature anisotropies in the WMAP Data
• Missing dust signature in the cosmic microwave background
• Cross-correlation analysis of CMB with foregrounds for residuals
• WMAP Polarization Results
• Trans-Planckian signals from the breaking of local Lorentz invariance
• Constraints on Cold Dark Matter in the Gamma-ray Halo of NGC 253
• Ellipticity of Structures in CMB Sky Maps
• Thermodynamics in Kaluza-Klein Universe
• Ray tracing the integrated Sachs-Wolfe effect through the light cones of the Dark Energy Universe Simulation -- Full Universe Runs
• Phantom shell around black hole and global geometry
• A new method to determine large scale structure from the luminosity distance
• A falsely fat curvaton with an observable running of the spectral tilt
• Quantum kinetic theory with nonlocal coherence
• Dynamics of Ferromagnetic Walls: Gravitational Properties
• Baryogenesis and CP-Violating Domain Walls in the Background of a Magnetic Field
• Power Spectra of CMB Polarization by Scattering in Clusters
• The interaction of extended Bose-Einstein condensate dark matter with viscous $f(T,B)$ gravity
• Gravito-magnetic gyroscope precession in Palatini f(R) gravity
• Testing for foreground residuals in the Planck foreground cleaned maps: A new method for designing confidence masks
• CMB Polarization as complementary information to anisotropies
• Local properties of the large-scale peaks of the CMB temperature
• A Viable Dark Fluid Model
• Inflationary scenario in the supersymmetric economical 3-3-1 model
• Refining the predictions of supersymmetric CP-violating models: A top-down approach
• Isocurvature Fluctuations Induce Early Star Formation
• Light Higgses and Dark Matter at Bottom and Charm Factories
• A Test for the Origin of Quasar Redshifts
• Cosmic Covariance and the Low Quadrupole Anisotropy of the Wilkinson Microwave Anisotropy Probe (WMAP) Data
• Cross-Correlation Studies with CMB Polarization Maps
• Non-singular model universe from a perfect fluid scalar-metric cosmology
• Exploring Supermassive Black Hole Growth with ALMA
• Estimation of spectrum and parameters of relic gravitational waves using space-borne interferometers
• Towards the optimal window for the 2MASS dipole
• Cosmic Sculpture: A new way to visualise the Cosmic Microwave Background
• Antimatter from the cosmological baryogenesis and the anisotropies and polarization of the CMB radiation
• Cosmological Magnetic Fields vs. CMB
• Braneworld inflation from an effective field theory after WMAP three-year data
• Dwarf Galaxies without Dark Matter: constraints on Modified Gravity
• Is there a common origin for the WMAP low multipole and for the ellipticity in BOOMERanG CMB maps?
• Lyman-alpha forest-CMB cross-correlation and the search for the ionized baryons at high redshift
• The Origin of the Large-Scale Structure in the Universe: Theoretical and Statistical Aspects
• What is the Cosmological Significance of a Discovery of Wimps at Colliders or in Direct Experiments?
• Lepton Flavour Violation in a Class of Lopsided SO(10) Models
• Extended Bose-Einstein condensate dark matter in viscous Gauss-Bonnet gravity
• De Sitter spacetimes with torsion in the model of dS gauge theory of gravity
• Observational Hubble parameter data constraints on the interactive model of $f(T)$ gravity with particle creation
• Fast, exact (but unstable) spin spherical harmonic transforms
• Observational Consequences of Quantum Cosmology
• Tachyon field inspired dark energy and supernovae constraints
• Correlation properties of the maps of the NVSS survey and WMAP ILC
• Resolving IRAS 09111-1007 at 350 microns - a different path to ULIRG formation?
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• Z-bursts from the Virgo cluster
• Holographic Dark Energy with Time Varying n^2 Parameter in Non-Flat Universe
• Dynamics of k-essence in loop quantum cosmology
• The issue of Dark Energy in String Theory
• DEMNUni: cross-correlating the nonlinear ISWRS effect with CMB-lensing and galaxies in the presence of massive neutrinos
• Neutralino annihilation beyond leading order
• CMB map restoration
• Constraining Parameters for the Accelerating Universe in $f(R,{\mathcal{L}}_m)$ Gravity
• Cosmological observations in non-local $F(R)$ cosmology
• Comparison of QG-Induced Dispersion with Standard Physics Effects
• Scalar quantities as detectors of non-Gaussianity on CMB maps
• Chandra Observation of the Interaction of the Radio Source and Cooling Core in Abell 2063
• Coupled inflaton and electromagnetic fields from Gravitoelectromagnetic Inflation with Lorentz and Feynman gauges
• Unveiling the Universe with Emerging Cosmological Probes
• Bayesian foreground analysis with CMB data
• Single Neutralino production at CERN LHC
• See-Saw Induced CMSSM Lepton-Flavour Violation Post-WMAP
• Baryogenesis: A Symmetry Breaking in the Primordial Universe Revisited
• Statistical and Observation Comparison of Weyl-Type $f(Q,T)$ Models with the $\Lambda$CDM Paradigm
• Is the physics within the Solar system really understood?
• Combining strongly lensed and unlensed fast radio bursts: To be a more precise late-universe probe
• Flow equations in generalized braneworld scenarios
• Forecast of foreground cleaning strategies for AliCPT-1
• Supermassive gravitinos, dark matter, leptogenesis and flat direction baryogenesis
• Dark Matter and Collider Phenomenology with two light Supersymmetric Higgs Bosons
• Hubble flow variations as a test for inhomogeneous cosmology
• A canonical formalism of f(T)-type gravity in terms of Lie derivatives
• Modified Teleparallel $f(T)$ Gravity, DESI BAO and the $H_0$ Tension
• Supersymmetric Heavy Higgses at e^+e^- Linear Collider and Dark-Matter Physics
• Eternally accelerating spacelike braneworld cosmologies
• Two-Component Cosmological Fluids with Gravitational Instabilities
• Anisotropic Dark Energy and the Generalized Second Law of Thermodynamics
• Constraining the Emission Properties of TeV Blazar H1426+428 by the Synchrotron-Self-Compton Model
• Some anisotropic universes in the presence of imperfect fluid coupling with spatial curvature
• An Axisymmetric Object-Based Search for a Flat Compact Dimension
• The model of a flat (Euclidean) expansive homogeneous and isotropic relativistic universe in the light of the general relativity, quantum mechanics, and observations
• Dirac Cosmology and the Acceleration of the Contemporary Universe
• Could the Lyra manifold be the hidden source of the dark energy?
• SUSY dark matter --A collider Physicist's Perspective--
• General Perfect Fluid Perturbations of Homogeneous and Orthogonal Locally Rotationally Symmetric Class II Cosmologies
• Cosmology in a supersymmetric model with gauged $B-L$
• New Inflation vs. Chaotic Inflation, Higher Degree Potentials and the Reconstruction Program in light of WMAP3
• Exact Polynomial Eigenmodes for Homogeneous Spherical 3-Manifolds
• Coincidence Problem in f(T) Gravity Models
• On a finite universe with no beginning or end
• A minimal set of invariants as a systematic approach to higher order gravity models: Physical and Cosmological Constraints
• A close examination of cosmic microwave background mirror-parity after Planck
• Second-order power spectra of CMB anisotropies due to primordial random perturbations in flat cosmological models
• An optimal system and invariant solutions of dark energy Models in cylindrically symmetric space-time
• Semiclassical Gravitoelectromagnetic inflation in a Lorentz gauge: seminal inflaton fluctuations and electromagnetic fields from a 5D vacuum state
• The primordial information content of Rayleigh Anisotropies
• VLA/JVLA Monitoring of Bright Northern Radio Sources
• MAGIC and the Search for Signatures of Supersymmetric Dark Matter
• Search for non-Gaussianities in the WMAP data with the Scaling Index Method
• New holographic Chaplygin gas model of dark energy
• Investigation of Bouncing Universe and Phantom Crossing in Modified Gravity Coupled with Weyl Tensor and its Reconstruction
• Dynamics of the self-interacting chameleon cosmology
• Palatini $f(\mathcal{R},{\mathcal{L}}_m,{\mathcal{R}}_{\mu \nu }{T}^{\mu \nu })$ gravity and its Born-Infeld semblance
• Observations of Galactic star-forming regions with the Cosmic Background Imager at 31 GHz
• Natural inflation in 5D warped backgrounds
• Semiclassical predictions regarding a pre-inflationary era and its effects on the power spectrum
• Domain walls in Born-Infeld-dilaton background
• Constraining the reionization history with large angle CMB polarization
• Curvaton Scenario in the Presence of Two Dilatons Coupled to the Scalar Curvature
• Dynamics of entropy perturbations in assisted dark energy with mixed kinetic terms
• The Bianchi type-V Dark Energy Cosmology in Self Interacting Brans Dicke Theory of Gravity
• Dynamics of Potentials in Bianchi Type Scalar-Tensor Cosmology
• Superluminal apparent motions in distant radio sources
• Status of the PICASSO Project
• Effects of particle creation rate in two-fluid interacting cosmologies
• Stochastic Gravity: Beyond Semiclassical Gravity
• QUIJOTE scientific results -- VI. The Haze as seen by QUIJOTE
• Long-lived Charginos in the Focus-point Region of the MSSM Parameter Space
• Neutrinos and the Phenomenology of CPT Violation
• Probing mSUGRA via the Extreme Universe Space Observatory
• Evolution of the Universe with Flat Extra Dimensions
• Weak Lensing Magnification Reconstruction with the Modified Internal Linear Combination Method
• Apparent versus true value of the cosmological constant
• Troubles for observing the inflaton potential
• Expansion-contraction duality breaking in a Planck-scale sensitive cosmological quantum simulator
• A Possible Late Time $\Lambda$CDM-like Background Cosmology in Relativistic MOND Theory
• Polarization of Sunyaev-Zeldovich signal due to electron pressure anisotropy in galaxy clusters
• Phantom Divide Crossing with General Non-minimal Kinetic Coupling
• Cosmological Perturbations During Radion Stabilization
• Time-Machines Construct in $f(\mathcal{R},\mathcal{A},A^{\mu \nu }{A}_{\mu \nu })$ and $f(\mathcal{R})$ Modified Gravity Theories
• A mechanism of the large-scale damping in the CMB anisotropy
• WMAP Bounds on Braneworld Tachyonic Inflation
• Suppression of the neutralino relic density with supersymmetric CP violation
• Astrometry meets Pulsar Timing Arrays: Synergies for Gravitational Wave Detection
• Indirect Detection of Kaluza-Klein Dark Matter from Latticized Universal Dimensions
• Correlating Fourier phase information with real-space higher order statistics
• Cosmological birefringence induced by neutrino current
• Few Body Reserch - Summary
• Cosmological parameters from Planck data in SU(2)${}_{\mathrm{CMB}}$, their local $\Lambda$CDM values, and the modified photon Boltzmann equation
• Statefinder analysis of the superfluid Chaplygin gas model
• Probing galaxy cluster and intra-cluster gas with luminous red galaxies
• Chameleon gravity on cosmological scales
• Space-time symmetry restoration in cosmological models with Kalb--Ramond and scalar fields
• Excess Ultraviolet Emission at High Galactic Latitudes: A New Horizons View
• Density perturbations from both the inflaton and the curvaton
• Interacting Kasner-type cosmologies
• Constraints on Field Theoretical Models for Variation of the Fine Structure Constant
• Are the WMAP angular magnification measurements consistent with an inhomogeneous critical density Universe?
• Signals of Inflation in a Friendly String Landscape
• Validity of Thermodynamical Laws in Dark Energy Filled Universe
• Long-Wavelength Modes of Cosmological Scalar Fields
• Testing synchrotron models and frequency resolution in BINGO 21 cm simulated maps using GNILC
• A Separate Universe Approach to Quintessence Perturbations
• Interacting Three Fluid System and Thermodynamics of the Universe Bounded by the Event Horizon
• The primordial non-Gaussianity of local type (f_NL) in the WMAP 5-year data: the length distribution of CMB skeleton
• Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions
• Phantom expansion with non-linear Schrödinger-type formulation of scalar field cosmology
• Kink instability and stabilization of the Friedmann universe with scalar fields
• Closed inflationary universe models in Braneworld Cosmology
• Dark matter in the MSSM and its singlet extension
• Multiscale analysis of the CMB temperature derivatives
• D/antiD Dark Energy in String Warped Compactification
• Eccentric inflation and WMAP
• Late-decaying Q-ball with BBN lifetime
• On the Absorption Properties of Metallic Needles
• Numerical Solutions of Inflating Higher Dimensional Global Defects
• Elements of dodecahedral cosmology
• On the Gravitational Field of Antimatter
• Absorption Variability of the Highly Obscured Active Galactic Nucleus NGC 4507
• A Thermal Graviton Background from Extra Dimensions
• Some studies on dark energy related problems
• The effect of supersymmetry breaking in the Mass Varying Neutrinos
• How accurately can suborbital experiments measure the CMB?
• Equation of State for Neutralino Star as a Form of Cold Dark Matter
• A very extended reionization epoch ?
• Accelerating behavior from dynamical system analysis parameters
• Predictions of Dynamically Emerging Brane Inflation Models
• The anomaly of the CMB power with the latest Planck data
• A Constrained NILC method for CMB B mode observations
• Long-Term X-Ray monitoring of NGC6251: Evidence for a jet-dominated radio galaxy
• Light Superpartners at Hadron Colliders
• Cosmic acceleration in a model of scalar-tensor gravitation
• Non-Gaussianity of the density distribution in accelerating universes
• On the wavelet analysis of CMB time ordered data: application to Archeops
• Stability analysis and observational constraints in scalar tensor theory
• Fine Tuning Problem of the Cosmological Constant in a Generalized Randall-Sundrum Model
• Dust Distribution during Reionization
• The obscured active nucleus of NGC 7172 as seen by NuSTAR
• Some effects of non-conservative gravity on cosmic string configurations
• The current problems of the minimal SO(10) GUT and their solutions
• Unified Gauge Theories and Reduction of Couplings: from Finiteness to Fuzzy Extra Dimensions
• Redshift estimation of clusters by wavelet decomposition of their Sunyaev-Zel'dovich morphology
• Bigravity: a bimetric model of the Universe with variable constants, inluding VSL (variable speed of light)
• Time Evolution of the Matter Content of the Expanding Universe in the Framework of Brans-Dicke Gravity
• A review of the stochastic background of gravitational waves in f(R) gravity with WMAP constrains
• A Scaling Relation in Inhomogeneous Cosmology with k-essence scalar fields
• Bulk scalar field in brane-worlds with induced gravity inspired by the $\mathcal{L}(R)$ term
• Significant foreground unrelated non-acoustic anisotropy on the one degree scale in WMAP 5-year observations
• Sky maps without anisotropies in the cosmic microwave background are a better fit to WMAP's uncalibrated time ordered data than the official sky maps
• Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe
• Discovery of a double ring in the dwarf galaxy Mrk409
• On Torsion-free Vacuum Solutions of the Model of de Sitter Gauge Theory of Gravity (II)
• The Thermal Sunyaev-Zeldovich Effect of Primordial Recombination Radiation
• Limiting Temperature, Limiting Curvature and the Cyclic Universe
• A Simple Gravitational Lens Model For Cosmic Voids
• Cosmic microwave background constraints on cosmological models with large-scale isotropy breaking
• Statefinder Diagnostic for Dark Energy Models in Bianchi I Universe
• Effective de Sitter brane via running radius
• Accretion of Holographic Dark Energy : Dependency only upon Horizon Radius of Expanding Universe
• Microwave Emission from the Edgeworth-Kuiper Belt and the Asteroid Belt Constrained from WMAP
• Can the CKM phase be the only source of CP violation?
• Modelling Cosmic Acceleration in Modified Yang - Mills Theory
• False Vacuum in the Supersymmetric Mass Varying Neutrinos Model
• Deconstructing the Cosmological Constant
• Dark Energy density in models with Split Supersymmetry and degenerate vacua
• Non-Minimal Cosmological Model in Modified Yang--Mills Theory
• Open Inflationary Universes in Gauss-Bonnet Brane Cosmology
• Statistics of WMAP ILC map temperature fluctuations towards distant radio galaxies
• Constraints on the primordial gravitational waves with variable sound speed from current CMB data
• The decoupling of scalar-modes from a linearly perturbed dust-filled Bianchi type I model
• Status and Perspectives of Neutrino Physics
• Neutrinos: Key to New Physics
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia, BAO, CMB, H(z) and X-ray gas mass fraction
• Level correlations of the CMB temperature angular power spectrum
• A Century of Cosmology
• Cosmological dynamics of D-cceleration
• A Solution to the Isolatitude, Equi-area, Hierarchical Pixel-Coordinate System
• Cosmic Acceleration from Causal Backreaction in a Smoothly Inhomogeneous Universe
• Phase Space Analysis for Anisotropic Universe with Nonlinear Bulk Viscosity
• Gravitational baryogenesis in $f(T,L_m)$ gravity
• Dark Energy Density in SUGRA models and degenerate vacua
• Fermion Scattering off a CP-violating Bubble Wall in the Background of a Uniform Magnetic Field
• Issues on the cosmological constant
• Beginning of Universe through large field hybrid inflation
• Entropy Production in the Inflationary Epoch Using the Gouy-Stodola Theorem
• Modified cosmology through generalized mass-to-horizon entropy: observational constraints from DESI DR2 BAO data
• Thermodynamics of the Primordial Universe
• The Energy Density of "Wound" Fields in a Toroidal Universe
• Spinflation from Geometric Tachyon
• Reflection Spectra of Accretion Disks Illuminated by an Off-Axis Corona
• Model Independent Foreground Power Spectrum Estimation using WMAP 5-year Data
• A model of cosmology and particle physics at an intermediate scale
• Optical properties of elongated conducting grains
• Density fluctuations on mm and Mpc scales
• Primordial vorticity and gradient expansion
• Cross-Correlation Detection of Point Sources in WMAP First Year Data
• Universality of Yukawa Couplings Confronts Recent Neutrino Data
• WMAP and Supergravity Inflationary Models
• Baryon asymmetry from higher-order matter contributions in gravity
• Protecting the primordial baryon asymmetry in the $SU(2{)}_L$ triplet Higgs model compatible with KamLAND and WMAP
• Probing Dark Energy Properties in $fQ,C)$ Gravity with FLRW Cosmological Models
• A Preposterous Universe
• Inflation and Leptogenesis in Five Dimensional SO(10)
• Baryon asymmetry constraints on Extended Symmetric Teleparallel Gravity
• Viscous interacting and stability on dark matter Bose-Einstein condensation with modified Chaplygin gas
• On accretion of dark energy onto black- and worm-holes
• Dynamical stability in scalar-tensor cosmology
• Forecasting 21-cm power spectrum sensitivity to dark Matter-baryon scattering
• Analytical analysis of the origin of core-cusp matter density distributions in galaxies
• Observational constraints on a Yang-Mills condensate dark energy model
• Constraints on Holographic cosmologies from strong lensing systems
• A New Contributor to Chemical Evolution in High-Redshift Galaxies
• D-bound and Bekenstein bound for McVittie solution surrounded by dark energy cosmological fields
• Foreground removal from WMAP 7yr polarization maps using an MLP neural network
• Bounding f(R,T) gravity by particle creation
• On Torsion-free Vacuum Solutions of the Model of de Sitter Gauge Theory of Gravity
• Agegraphic dark energy with the sign-changeable interaction in non-flat universe
• A Kaluza-Klein Inspired Brans-Dicke Gravity with Dark Matter and Dark Energy Model
• Instability Analysis of Cylindrical Stellar Object in Brans-Dicke Gravity
• Determining the Actual Local Density of Dark Matter Particles
• Reconstruction of the One-point Distribution of Convergence from Weak Lensing by Large-scale Structure
• Phase structure of the $O(2)$ ghost model with higher-order gradient term
• Tantalizing New Physics from the Cosmic Purview
• Globular clusters as cosmic clocks: new cosmological hints from their integrated light
• Cosmological Evolution of Viscous Dark Energy in f(Q,C) Gravity: Two-Fluid Approach
• Non-gaussianity and Statistical Anisotropy in Cosmological Inflationary Models
• Conformally de Sitter space from anisotropic SD3-brane of type IIB string theory
• Tuning the stochastic background of gravitational waves using the WMAP data
• Diagnosing Timing Error in WMAP Data
• Can MONDian vector theories explain the cosmic speed up ?
• The Cosmic Microwave Background anisotropies: open problems
• Cosmological constraints from galaxy clustering
• Asymptotically Static Universe
• Quadrant asymmetry in the angular distribution of the Cosmic Microwave Background in the Planck satellite data
• Embedded Lensing Time Delays, the Fermat Potential, and the Integrated Sachs-Wolfe Effect
• Predicting the Polarization of The Microwave Background from the WMAP Temperature Maps
• Sensitivity and Insensitivity of Galaxy Cluster Surveys to New Physics
• Excess ellipticity of hot and cold spots in the WMAP data?
• Global Spectral Energy Distributions of the Large Magellanic Cloud with Interstellar Dust
• Supersymmetric dark energy
• A Holographic Energy Model
• Cosmological constraints from Gauss-Bonnet braneworld with large-field potentials
• Cyclotron emission effect on CMB spectral distortions
• CMB likelihood approximation for banded probability distributions
• Space-like Dp branes: accelerating cosmologies versus conformally de Sitter space-time
• Gamma rays from dark matter annihilation in the Draco and observability at ARGO
• Dark Matter Constituents
• G-corrected holographic dark energy model
• Cosmological Constant Probing Shape Moduli through Large Extra Dimensions
• Constraints on the Sum of Neutrino Masses from Cosmology and their impact on world neutrino data
• Self-supervised component separation for the extragalactic submillimeter sky
• Investigation of Possible Dark Matter Direct Detection in Electron Accelerators
• On asymptotic behavior of anisotropic Dvali-Gabadadze-Porrati branes
• Characterizing the equivalence between dark energy and radiation using gamma-ray bursts
• Domain Wall and Holographic Dark Energy in $f(Q)$ Theory of Gravity
• Neutrino Data, CP violation and Cosmological Implications
• Complexity in cosmic structures
• Parameter estimation for a Lorentz invariance violation
• Cosmic microwave background limits on spatially homogeneous cosmological models with dark energy
• Variations of the Fine Structure Constant in Space and Time
• Complex supergravity quintessence models confronted with Sn Ia data
• Development of the Universe and New Cosmology
• Sterile Neutrinos in astrophysical and cosmological sauce
• Cosmic String Wake Detection using 3D Ridgelet Transformations
• Anisotropic cosmology using observational datasets: exploring via machine learning approaches
• Viscous fluid dynamics with decaying vacuum energy density
• kSZ Pairwise Velocity Reconstruction with Machine Learning
• Observational constraints in scalar tensor theory with tachyonic potential
• An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$
• Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements
• Application of Genetic Algorithm to Estimate the Large Angular Scale Features of Cosmic Microwave Background
• CMB Anomalies from Imperfect Dark Energy: Confrontation with the Data
• CMB B-mode polarization from Thomson scattering in the local universe
• Renormalizable minimal SO(10) GUT in 4D and 5D
• Primordial non-Gaussianity estimator: the inhomogeneous noise effect
• Dark matter, dark energy and modern cosmology: the case for a Kuhnian paradigm shift
• Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors
• Isotropy in the two-point angular correlation function of the CMB
• Dynamics of inflationary cosmology in TVSD model
• Electroweak Precision Data and Gravitino Dark Matter
• Systematic effects induced by a flat isotropic dielectric slab
• Soft X-ray excess of clusters: a thermal filament model, and the strong lensing of background galaxy groups
• Protecting the primordial baryon asymmetry in the seesaw model compatible with WMAP and KamLAND
• Method of determining cosmological parameter ranges with samples of candles with an intrinsic distribution
• A model of inflation independent of the initial conditions, with bounded number of e-folds and n_s larger orsmaller than one
• Zonal Modes of Cosmic Microwave Background Temperature Maps
• Theory and Phenomenology of Dirac Leptogenesis
• Nearly Full-Sky Low-Multipole Cosmic Microwave Background Temperature Anisotropy: III. CMB Temperature Anomalies
• Leptogenesis in a seesaw model with Fritzsch type lepton mass matrices
• Unified first law for traversable wormholes in non-minimal coupling of curvature and matter
• The two-and three-point correlation functions of the polarized five-year WMAP sky maps
• Cosmic Microwave Background Polarization
• Simulations of cm-wavelength Sunyaev-Zel'dovich galaxy cluster and point source blind sky surveys and predictions for the RT32/OCRA-f and the Hevelius 100-m radio telescope
• Observational constraints on models of the Universe with time variable Gravitational and Cosmological constants along MOG
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• Conjecture on the Avoidance of the Big Crunch
• AdSS_5 Brane World Cosmology
• Constraints on scalar-tensor theories from observations
• Topological Zero-Thickness Cosmic Strings
• LHC / ILC / Cosmology Interplay
• Particle Dark Matter from Physics Beyond the Standard Model
• Nearly Full-Sky Low-Multipole Cosmic Microwave Temperature Anisotropy: I. Foreground Cleaned Maps
• "Bimaximal + Democratic" type neutrino mass matrix in view of quark-lepton complementarity
• A Relativistic Scalar Model for Fractional Interaction between Dark Matter and Gravity
• Revisiting Ryskin's Model of Cosmic Acceleration
• Models for the Clustering of Far-Infrared and Sub-millimetre selected Galaxies
• Time evolution of a non-singular primordial black hole
• Tools for Dark Matter in Particle and Astroparticle Physics
• New Constraints on Dark Energy
• The Contribution of Novel CP Violating Operators to the nEDM using Lattice QCD
• Vacuum Energy Density and Cosmological Constant in dS Brane World
• Scalar-induced gravitational waves including isocurvature perturbations with lattice simulations
• String Imprints from a Pre-inflationary Era
• Constraining the primordial power spectrum using a differentiable likelihood
• Next-generation test of cosmic inflation
• The WSRT virgo filament survey
• The interplay between high energy physics and cosmology: an example
• An exact result concerning the $1/f$ noise contribution to the large-angle error in CMB temperature and polarization maps
• Cosmological principle and honeycombs
• Gravitational Effects of Varying Alpha Strings
• Exact solution and exotic fluid in cosmology
• Theory of Cosmological Perturbations and Applications to Superstring Cosmology
• Do JWST reionization (optical depth) puzzle, cosmological tensions, and CMB anomalies imply Harrison-Zel'dovich spectrum?
• Flat-Directions in Grand Unification With $U(1{)}_R$ Symmetry
• Thermal leptogenesis in a 5D split fermion scenario with bulk neutrinos
• Black Strings in Our World
• Crossing the phantom divide with k-essence in brane-worlds
• A cosmological test for general relativity
• Can galactic magnetic fields diffuse into the voids?
• On the nature of the first galaxies selected at 350 microns
• Scalar-tensor baryogenesis: a scalar-tensor completion of gravitational baryogenesis
• Initial Condition of Relic Gravitational Waves Constrained by LIGO S6 and Multiple Interferometers
• Gravitational collapse disturbs the dS/CFT correspondence?
• Homology reveals significant anisotropy in the cosmic microwave background
• An inhomogeneous universe with thick shells and without cosmological constant
• Li isotopes in metal-poor halo dwarfs, a more and more complicated story
• WMAP constraint on the P-term inflationary model
• Unplugging the Universe: the neglected electromagnetic consequence of decoupling
• Ultra-compact Objects of Non-minimally Coupled Dark Matter
• CP violation in bilinear R-parity violation and its consequences for the early universe
• Clarifying Inflation Models: the Precise Inflationary Potential from Effective Field Theory and the WMAP data
• CMB low multipole alignments across WMAP and \emph{Planck} data releases
• Modified cosmology through generalized mass-to-horizon entropy: implications for structure growth and primordial gravitational waves
• The COSMOS Wall at z$\sim$0.73: star-forming galaxies and their evolution in different environments
• A new single-dynamical-scalar-field model of dark energy
• Interacting Models of Generalised Chaplygin Gas and Modified Chaplygin Gas with Barotropic Fluid
• Stochastic stabilization of cosmological photons
• Vacuum energy and Primordial Black Holes in Brans-Dicke Theory
• Looking for the Signals of the Missing Baryons in the Extragalactic Background Light
• Parameter estimation of eccentric massive black hole binaries with LISA and its cosmological implications
• Proposal for Generic Size of Large Extra Dimensions
• Cyclic Universe à la string theory
• Theoretical priors in scalar-tensor cosmologies: Shift-symmetric Horndeski models
• Cosmology of Einstein-Vlasov system in a weak modification of general relativity
• Relativity principle with a low energy invariant scale
• Argument for the radiation-dominated behavior of matter fields in the preinflationary era
• Dark energy from conformal symmetry breaking
• Modular Invariant Soft Breaking, WMAP, Dark Matter and Sparticle Mass Limits
• Gradient measure and extended self-similarity of the cosmic microwave background anisotropy
• A non-singular closed bouncing universe without violation of null energy condition
• The possibility of a stable flat dark energy-dominated Swiss-cheese Brane-world universe with a deceleration-acceleration transition
• Dark Energy Density in Brane World
• Dark matter and Modified Newtonian Dynamics in a sample of high-redshift galaxy clusters observed with Chandra
• Constrain intergalactic medium from the SZ effect map
• Gravity and induced matter on Nearly Kahler Manifolds
• A Relativistic Tensorial Model for Fractional Interaction between Dark Matter and Gravity
• Are dark matter and dark energy omnipresent?
• Cosmology with CMB anisotropy
• Power Suppression and Lensing Anomaly -- A phenomenological investigation
• Cluster optical depth and pairwise velocity estimation using machine learning
• Pico: Parameters for the Impatient Cosmologist
• Falsifying Tree Level String Motivated Bouncing Cosmologies
• Gravitational baryogenesis of cosmological constant dominated universe
• Transverse Momentum Correlations in Relativistic Nuclear Collisions
• A Cyclic Cosmological Model in the Landscape Scenario
• Cosmic Acceleration Caused by the Extra-Dimensional Evolution in a Generalized Randall-Sundrum Model
• $d{S}_4$ vacua from matter-coupled 4D N=4 gauged supergravity
• $d{S}_5$ vacua from matter-coupled 5D N=4 gauged supergravity
• Stochastic gravitational wave from graviton bremsstrahlung in inflaton decay into massive spin 3/2 particles
• Cosmological model with Born-Infeld type scalar field
• Non-Gaussianity of the density distribution in accelerating universes II:N-body simulations
• Warm inflation in Weyl geometric gravity
• Angular Power Spectrum in Modular Invariant Inflation Model
• Cosmic Microwave Background anisotropies: the power spectrum and beyond
• Revisiting Agegraphic Dark Energy in Brans-Dicke Cosmology
• Raising Sfermion Masses by Adding Extra Matter Fields
• Foreground removal in HI 21 cm intensity mapping under frequency-dependent beam distortions
• Cosmological solutions for model with a $1/H^2$ term
• The Ligo-Ligo cross correlation for the detection of relic scalar gravitational waves
• Leptonic CP Violation and Leptogenesis
• Competition Between Gravitational and Scalar Field Radiation
• Can hyperbolic phase of Brans-Dicke field account for Dark Matter?
• Correspondence between modified gravity and 5D Ricci-flat cosmologies
• Edwards-Wilkinson surface over a spherical substrate: $1/f$ noise in the height fluctuations
• Constraining the mSUGRA parameter space using the entropy of dark matter halos
• Spherical Gravitational Collapse of Annihilating Dark Matter and the Minimum Mass of CDM Black Holes
• High Energy Neutrinos as a Probe for New Physics and Astrophysics
• Tachyonic Universes in Patch Cosmologies with $\Omega >1$
• Cosmological Constraints on the Undulant Universe
• A Study on the Expanding Universe Based on a Model of the Time Variation of its Matter Content in the Framework of Brans-Dicke Theory
• Dynamical modelling of the elliptical galaxy NGC 2974
• On Cosmological Low Entropy After the Big Bang: Universal Expansion and Nucleosynthesis
• Hidden in the background: a local approach to CMB anomalies
• A non-singular universe with vacuum energy
• A new approach to modified-gravity models
• The Dirac equation in the Kerr-de Sitter metric
• Accelerating Kaluza-Klein Universe in Modified Theory of Gravitation
• Bianchi type-III THDE quintessence model with hybrid expansion law
• Inflation and Generalized O'Raifeartaigh SUSY models
• Top and Bottom Squarks Decays under Cosmological Bounds
• Baryogenesis in Brans-Dicke theory
• Energy composition of the Universe: time-independent internal symmetry
• On the smallness of the cosmological constant
• Non-Gaussianities in the local curvature of the 5-year WMAP data
• A toy model for the coincidence problem
• Semi-holographic model revisited
• Acceleration of the universe in matter dominant era by conformal symmetry breaking
• Generalized Second Law of Thermodynamics on the Event Horizon for Interacting Dark Energy
• Evolution of cosmological event horizons in anisotropic universes
• The small mixing angle ${\theta }_{13}$ and the lepton asymmetry
• Present and future prospects for lattice QCD calculations of matrix elements for nEDM
• An accelerated closed universe
• The Ku-band Polarization Identifier
• On Topological Defects and Cosmological Constant
• Reproducing neutrino effects on the matter power spectrum through a degenerate Fermi gas approach
• A characterization of the diffuse Galactic emissions in the anti-center of the Galaxy
• Tensorial Quantum Gravity and the Cosmological Constant Problem
• Self Creation Cosmology - An Alternative Gravitational Theory
• Evolution of the horizons for dark energy universe
• Constraining Planck scale physics with CMB and Reionization Optical Depth
• Supersymmetry Searches at the LHC
• The MSSM with Non-Universal Higgs Masses
• Long-wavelength gravitational waves and cosmic acceleration
• Static, Cylindrically Symmetric Spacetimes in the Coincident f(Q) Gravity
• Optimal Extraction of Cosmological Information from Supernova Data in the Presence of Calibration Uncertainties
• An Oscillating Holographic Dark Energy in $f(R)$ Gravity
• Geometric and thermodynamic properties in Gauss-Bonnet gravity
• Searching for Neutrinos from WIMP Annihilations in the Galactic Stellar Disk
• Conservation of nonlinear curvature perturbations on super-Hubble scales
• Inflation with the Trace Anomaly Action and Primordial Black Holes
• Sunyaev-Zeldovich Cluster Counts as a Probe of Intra-Supercluster Gas
• Charged anisotropic white dwarfs in $f\left(R,T\right)$ gravity
• Squark Decays in MSSM Under the Cosmological Bounds
• Non-Gaussianity in Cosmology: from Inflation to the CMB
• Do We Live in a Vanilla Universe? Theoretical Perspectives on WMAP
• de Vaucouleurs-Ikeuchi Diagram and Commutation Relations among Phase Space Coordinates
• A new approach for constraining the Hubble constant from proper motions of radio jets
• `Standard' Cosmological model & beyond with CMB
• Radiation dominated era and the power of general relativity
• Higgs-Boson Benchmarks in Agreement with CDM, EWPO and BPO
• The Mass Function of Dark Matter Haloes in a Cosmological Model with a Running Primordial Power Spectrum
• Nonlinear Spinor Fields in LRS Bianchi type-I spacetime: Theory and observation
• Self-restriction of Gravitational Field and its Role in the Universe
• Cosmological quests in the CMB sky
• Axion boson stars with wormhole topology
• Neutrino Physics and CP violation
• 25 years of Cosmic Microwave Background research at INPE
• Gauge Field Theory of Horizontal Symmetry Generated by a Central Extension of the Pauli Algebra
• Testing SUGRA Models
• Too Early? On the Apparent Conflict of Astrobiology and Cosmology
• Noether symmetry of FRW cosmology with f - essence
• Numerical Correpondences between the physical Constants
• Galactic Plane image sharpness as a check on cosmic microwave background mapmaking
• Radiative Symmetry Breaking in the Supersymmetric Minimal B-L Extended Standard Model
• A window to quantum gravity phenomena in the emergence of the seeds of cosmic structure
• Constraining Post-Newtonian f(R) Gravity in the Solar System
• Mimicking two field inflationary features with a single field
• Implications of correlations and fluctuations in small systems
• Constraints on lepton flavour violation and leptogenesis
• Seeable universe and its accelerated expansion: an observational test
• Limits on the integration constant of the dark radiation term in Brane Cosmology
• Probability of Creation of Extra Dimensions in Nuclear Collisions
• CMB line-of-sight integrators for nearly-isotropic cosmological models
• Accelerating Cosmologies with Extended Product Spaces
• Large Number, Dark Matter, Dark Energy, and the Superstructures in the Universe (with Extension)
• Non Thermal Features in the Cosmic Neutrino Background
• Cosmological Model of Interacting Phantom and Yang-Mills Fields
• A New Fast Parallel Statistical Measurement Technique for Computational Cosmology
• Correspondence between particle creation and dark components interaction in the context of $f(\mathcal{G})$ gravity
• Can accelerated expansion of the universe be due to spacetime vorticity?
• On curvature coupling and quintessence fine-tuning
• Lost Baryons at Low Redshift
• The Kaiser-Rocket effect: three decades and counting
• Mapping the dark matter using weak lensing
• On Gauge Choice of Spherically Symmetric 3-Branes
• Interplay of Electroweak Precision Observables and B Physics Observables
• A halo approach to the evaluation of the cross-correlation between the SZ sky and galaxy survey
• Phase space analysis of Rényi Holographic dark energy model
• An Open Inflationary Model for Dimensional Reduction and its Effects on the Observable Parameters of the Universe
• Chandra and FUSE view of the WHIM: the Local Group and beyond
• Contrasting evolutionary pathways of fast- and slow-rotating galaxies in the green valley
• Mori-Zwanzig formalism for early cosmic inflation
• Gravitational Structure Formation, the Cosmological Problem and Statistical Physics
• Nonlinear Lattice Framework for Inflation: Bridging stochastic inflation and the $\delta N$ formalism
• Is there a chance that the anisotropies in the cosmic microwave background detected by COBE are an artefact of COBE's image reconstruction?
• Topics in Cosmology
• Observational Constraints and Geometric Diagnostics of Barboza-Alcaniz and Logarithmic Dark Energy Parametrizations
• Cosmic chronometers with galaxy clusters: a new avenue for multi-probe cosmology
• Looking Beyond Inflationary Cosmology
• Probing Reionization with the Cosmological Proximity Effect and High-Redshift Supernovae Rates
• Intracluster Medium through three years of WMAP
• Exploring trans-Planckian physics and the curvature effect by primordial power spectrum with WMAP five-year data
• Anisotropic evolution of D-dimensional FRW spacetime
• CMB Observational Techniques and Recent Results
• Some Consequences of Dark Energy Density varying Exponentially with Scale Factor
• Relation between CKM and MNS Matrices Induced by Bi-Maximal Rotations in the Seesaw Mechanism
• Evidence of Heavy Obscuration in the Low-Luminosity AGN NGC 4941
• BrahMap: A scalable and modular map-making framework for the CMB experiments
• Summary of ICGC04 Cosmology Workshop
• Large-Angle Anomalies in the Microwave Background
• Deconstructing Functions on Quadratic Surfaces into Multipoles
• A characterization of the diffuse Galactic emissions at large angular scales using the Tenerife data
• Numerical study of leptogenesis in a 5D split fermion model with bulk neutrinos
• Is the Pre-WMAP CMB Data Self-consistent?
• Testing the effects from dark radiation
• Searches for Cosmic Antimatter
• Maps of the Cosmos: The Cosmic Microwave Background
• A possible explanation for NuTeV's anomalous dimuon events
• WHIM emission and the cluster soft excess: a model comparison
• Asymmetry and non-random orientation of the inflight effective beam pattern in the WMAP Data
• Generalized Milne Space, Eternal Accelerating Cosmology, Ep-branes and dS/CFT Correspondence
• Probing Neutrino low energy and mass scales
• Cosmological models with the spinor and non-minimally interacting scalar field
• A multiwavelength study of near- and mid-infrared selected galaxies at high redshift: ERGs, AGN-identification and the contribution from dust
• A Tempt To Measure Reality
• Producing and constraining self-interacting hidden sector dark matter