A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation

Abstract

The blackbody radiation left over from the Big Bang has been transformed by the expansion of the Universe into the nearly isotropic 2.73K Cosmic Microwave Background. Tiny inhomogeneities in the early Universe left their imprint on the microwave background in the form of small anisotropies in its temperature. These anisotropies contain information about basic cosmological parameters, particularly the total energy density and curvature of the universe. Here we report the first images of resolved structure in the microwave background anisotropies over a significant part of the sky. Maps at four frequencies clearly distinguish the microwave background from foreground emission. We compute the angular power spectrum of the microwave background, and find a peak at Legendre multipole ${\ell }_{peak}=(197\pm 6)$, with an amplitude $D{T}_{200}=(69\pm 8)\mu K$. This is consistent with that expected for cold dark matter models in a flat (euclidean) Universe, as favoured by standard inflationary scenarios.

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• Physics of dark energy particles
• SO(1,1) dark energy model and the universe transition
• An Interacting Two-Fluid Scenario for Dark Energy in FRW Universe
• Archeops: A High Resolution, Large Sky Coverage Balloon Experiment for Mapping CMB Anisotropies
• Cosmology in scalar tensor theory and asymptotically de-Sitter Universe
• New measurements of ${\Omega }_m$ from gamma-ray bursts
• Gravitational Wave Background from Magnetars
• Interacting new agegraphic dark energy in non-flat Brans-Dicke cosmology
• The Weak Lensing Radial Acceleration Relation: Constraining Modified Gravity and Cold Dark Matter theories with KiDS-1000
• Tsallis holographic dark energy in the brane cosmology
• Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• Friedmann's Equations in All Dimensions and Chebyshev's Theorem
• Superposition of blackbodies and the dipole anisotropy: A possibility to calibrate CMB experiments
• Aspects of the Cosmic Microwave Background Dipole
• Generalized Chaplygin Gas Models tested with SNIa
• Can Supersymmetry Naturally Explain the Positron Excess?
• ROMA: a map-making algorithm for polarised CMB data sets
• A model of the Universe including Dark Energy accounted for by both a Quintessence Field and a (negative) Cosmological Constant
• Cosmic Background of Gravitational Waves from Rotating Neutron Stars
• BOOMERanG Data Suggest a Purely Baryonic Universe
• New Constraints on inflation from the Cosmic Microwave Background
• Interacting Ghost Dark Energy in Brans-Dicke Theory
• Classical and Quantum Features of the Mixmaster Singularity
• Fast Pixel Space Convolution for CMB Surveys with Asymmetric Beams and Complex Scan Strategies: FEBeCoP
• Kinetic k-essence ghost dark energy model
• A needlet ILC analysis of WMAP 9-year polarisation data: CMB polarisation power spectra
• Future Universe With w < -1 Without Big Smash
• Dark energy and particle mixing
• Making sky maps from Planck data
• Measuring the properties of extragalactic dust and implications for the Hubble diagram
• Nonvanishing Cosmological Constant of Flat Universe in Brane-World Scenario
• Eternal Inflation
• Emergent Universe Scenario in the Einstein-Gauss-Bonnet Gravity with Dilaton
• New inflation in supergravity with a chaotic initial condition
• Non-Gaussian Aspects of Thermal and Kinetic Sunyaev-Zel'dovich Effects
• The Impact of Cosmic Dust on Supernova Cosmology
• Topology of structure in the Sloan Digital Sky Survey: model testing
• Self-interacting dark matter from an SU(3)_L \otimes U(1)_N electroweak model
• Astronomy in Antarctica
• Constraining Van der Waals quintessence by observations
• Reconstructing f(R) modified gravity from ordinary and entropy-corrected versions of the holographic and new agegraphic dark energy models
• New constraints on neutrino physics from Boomerang data
• Barrow black hole corrected-entropy model and Tsallis nonextensivity
• Combining maximum-entropy and the mexican hat wavelet to reconstruct the microwave sky
• Models of dark matter halos based on statistical mechanics: I. The classical King model
• The local Hubble flow: a manifestation of dark energy
• Supernova constraints on decaying vacuum cosmology
• Phase space geometry in scalar-tensor cosmology
• Density Perturbations for Running Cosmological Constant
• A Running Spectral Index in Supersymmetric Dark-Matter Models with Quasi-Stable Charged Particles
• Scale Dependent Spectral Index in Slow Roll Inflation
• Precision cosmology with a wide area XMM cluster survey
• Limits on Supersymmetric Dark Matter From EGRET Observations of the Galactic Center Region
• Interacting new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe
• SN and BAO constraints on (new) polynomial dark energy parametrizations: current results and forecasts
• The 2dF Galaxy Redshift Survey: constraints on cosmic star-formation history from the cosmic spectrum
• Time-delay cosmographic forecasts with strong lensing and JWST stellar kinematics
• Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters
• Sterile neutrinos: direct mixing effects versus induced mass matrix of active neutrinos
• Maximum Likelihood Estimates of the Two- and Three-Dimensional Power Spectra of the APM Galaxy Survey
• Accelerating dark energy models in bianchi Type-V space-time
• Cosmological Perturbations with Multiple Scalar Fields
• Towards a Precision Cosmology from Starburst Galaxies at z>2
• Support of dS/CFT correspondence from space-time perturbations
• CMB Temperature and Polarization Anisotropy Fundamentals
• Big smash of the universe
• Cross-Correlation of the Cosmic Microwave Background with Radio Sources: Constraints on an Accelerating Universe
• Supersymmetric Theories of Neutrino Dark Energy
• Neutralino Dark Matter Elastic Scattering in a Flat and Accelerating Universe
• O(N) quintessence
• Phantom appearance of non-phantom matter
• Removing 1/f noise stripes in cosmic microwave background anisotropy observations
• The generalized second law of gravitational thermodynamics on the apparent and event horizons in FRW cosmology
• Testing Standard and Degenerate Big Bang Nucleosynthesis with BOOMERanG and MAXIMA-1
• Weak Lensing of the CMB: Extraction of Lensing Information from the Trispectrum
• Multiple Methods for Estimating the Bispectrum of the Cosmic Microwave Background with Application to the MAXIMA Data
• Does the cosmological constant imply the existence of a minimum mass?
• Study of gravastars under $f(\mathbb{T})$ gravity
• Holographic f(T)-gravity model with power-law entropy correction
• Remarks on the formulation of the cosmological constant/dark energy problems
• The CMB temperature power spectrum from an improved analysis of the Archeops data
• Fitting Type Ia supernovae with coupled dark energy
• Direct and Indirect Detection of Neutralino Dark Matter In Selected Supersymmetry Breaking Scenarios
• Assisting pre-big bang phenomenology through short-lived axions
• Chandra X-Ray Observatory Observation of the High-Redshift Cluster MS 1054-0321
• Constraints on inflation from CMB and Lyman-alpha forest
• The Host Galaxy and Optical Light Curve of the Gamma-Ray Burst GRB 980703
• Constraining the expansion rate of the Universe using low-redshift ellipticals as cosmic chronometers
• Casimir energy-momentum tensor for a brane in de Sitter spacetime
• Restframe I-band Hubble diagram for type Ia supernovae up to redshift z ~0.5
• Metallicity Evolution of Damped Lyman Alpha Systems In Lambda CDM Cosmology
• Stellar Archaeology: a Keck Pilot Program on Extremely Metal-Poor Stars From the Hamburg/ESO Survey. I Stellar Parameters
• Extended quintessence and the primordial helium abundance
• Cosmological implications of APM 08279+5255, an old quasar at z = 3.91
• The Road to Precision Cosmology
• Inflation and non--Gaussianity
• Condensate cosmology -- dark energy from dark matter
• Systematic biases on galaxy haloes parameters from Yukawa-like gravitational potentials
• Extended Quintessence and its Late-time Domination
• An alternative to the LCDM model: the case of scale invariance
• Predictions and Observations in Theories with Varying Couplings
• Evolution of density perturbations in decaying vacuum cosmology
• The missing link: a nonlinear post-Friedmann framework for small and large scales
• Search for non-gaussian signals in the BOOMERanG maps: pixel-space analysis
• Quintessence, Cosmology, and Fanaroff-Riley Type IIB Radio Galaxies
• Massive Charged Scalar Quasinormal Modes of Reissner-Nördstrom Black Hole Surrounded by Quintessence
• One Hundred Years of the Cosmological Constant: from 'Superfluous Stunt' to Dark Energy
• The signature of dark energy on the local Hubble flow
• Dark Matter and Dark Energy from the solution of the strong CP problem
• Confrontation of MOND Predictions with WMAP First Year Data
• The Angular Power Spectrum of EDSGC Galaxies
• Late time cosmological approach in mimetic $f(R,T)$ gravity
• High-resolution asymptotics for the angular bispectrum of spherical random fields
• Interacting entropy-corrected new agegraphic dark energy in Brans-Dicke cosmology
• Existence of bulk viscous universe in $f(R,T)$ gravity and confrontation with observational data
• The redshift determination of GRB 990506 and GRB 000418 with the Echellete Spectrograph Imager on Keck
• The generalized second law in irreversible thermodynamics for the interacting dark energy in a non-flat FRW universe enclosed by the apparent horizon
• Buchdahl model in f(R, T) gravity: A comparative study with standard Einstein's gravity
• Constraints on Cardassian Scenario from the Expansion Turnaround Redshift and the Sunyaev-Zeldovich/X-ray Data
• Gravastars in $f(R,G)$ Gravity
• Holographic dark energy in Brans-Dicke theory with log correction
• Oscillations in the dark energy EoS: new MCMC lessons
• Quantitative evolution of global strings from the Lagrangian viewpoint
• Constraining Fundamental Physics with Future CMB Experiments
• Acceleration of the universe, vacuum metamorphosis, and the large-time asymptotic form of the heat kernel
• Accelerating Universe in Hybrid and Logarithmic Teleparallel Gravity
• Gravitational lensing in modified Newtonian dynamics
• Remarks on the Boomerang results, the baryon density and the leptonic asymmetry
• Can Quintessence Be The Rolling Tachyon?
• Varying G, accelerating Universe, and other relevant consequences of a Stochastic Self-Similar and Fractal Universe
• Cosmological Parameters from Velocities, CMB and Supernovae
• Cosmic accelerated expansion and the entropy corrected holographic dark energy
• Bayesian Evidence against Harrison-Zel'dovich spectrum in tension cosmology
• Characterising the Primordial Cosmic Perturbations
• Palatini formulation of the $R^{-1}$modified gravity with an additionally squared scalar curvature term
• Large Scale Structure
• CMB constraints on interacting cosmological models
• A simple nonsingular inflationary quintessential model
• Uniqueness of the Fock quantization of scalar fields in spatially flat cosmological spacetimes
• The QMAP and MAT/TOCO Experiments for Measuring Anisotropy in the Cosmic Microwave Background
• A 3-D model of polarised dust emission in the Milky Way
• ADM formulation and Hamiltonian analysis of $f(Q)$ gravity
• Charged Gravastars with Conformal Motion in f(R,T) Gravity
• The Cosmic Microwave Background: The history of its experimental investigation and its significance for cosmology
• A Supernova Brane Scan
• Viscous dissipative Chaplygin gas dominated homogenous and isotropic cosmological models
• Viscous dark energy and generalized second law of thermodynamics
• Constraining f(T) gravity by dynamical system analysis
• Is the evidence for dark energy secure?
• Asymmetric Beams in Cosmic Microwave Background Anisotropy Experiments
• What is the best way to measure baryonic acoustic oscillations?
• The radio source counts at 15 GHz and their implications for cm-wave CMB imaging
• Mass-Temperature Relation of Galaxy Clusters: A Theoretical Study
• Matrix Model for De Sitter
• Holographic Discreteness of Inflationary Perturbations
• Dark matter as a Weyl geometric effect
• Spatial Variation of the Fine-Structure Parameter and the Cosmic Microwave Background
• Supernova constraints on alternative models to dark energy
• Study of Gravastars in Rastall Gravity
• The Scale of Cosmic Isotropy
• One-loop f(R) Gravitational Modified Models
• Natural Double Inflation in Supergravity
• Secondary CMB Anisotropies from Cosmological Reionization
• Observational constraints on dark energy model
• How to fool CMB parameter estimation
• Dark energy model with variable $q$ and $\omega$ in LRS Bianchi-II space-time
• On the Degeneracy Inherent in Observational Determination of the Dark Energy Equation of State
• Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in non-flat universe
• Holographic Dark Energy and the Universe Expansion Acceleration
• Update of the direct detection of dark matter and the role of the nuclear spin
• QUBIC I: Overview and ScienceProgram
• Matching the observational value of the cosmological constant
• Age constraints on the cosmic equation of state
• Cosmological non-Gaussian Signature Detection: Comparing Performance of Different Statistical Tests
• Supernova data may be unable to distinguish between quintessence and k-essence
• Ionization history of the cosmic plasma in the light of the recent CBI and future PLANCK data
• Testing Cosmology with Cosmic Sound Waves
• Evolutionary behaviour of cosmological parameters with dynamical system analysis in f (Q, T) gravity
• Dark energy with polytropic equation of state
• High latitude Galactic dust emission in the BOOMERanG maps
• Dark energy and the epoch of galaxy formation
• Back-Reaction Is For Real
• Has the Universe always expanded ?
• Thermodynamics of apparent horizon in modified FRW universe with power-law corrected entropy
• The Long-Term Future of Extragalactic Astronomy
• Method for Direct Measurement of Cosmic Acceleration by 21-cm Absorption Systems
• The inflationary gravitational-wave background and measurements of the scalar spectral index
• Emergent physics: Fermi point scenario
• Hidden past of dark energy cosmological models
• Reconstruction of f(T) and f(R) gravity according to (m,n)-type holographic dark energy
• Accelerating dark energy models with anisotropic fluid in Bianchi type-$V{I}_0$ space-time
• Unbiased Estimate of Dark Energy Density from Type Ia Supernova Data
• Present Acceleration of Universe, Holographic Dark Energy and Brans-Dicke Theory
• Cluster Formation Rate in Models with Dark Energy
• Generation of cosmological large lepton asymmetry from a rolling scalar field
• Unimodular $f(R,T)$ Gravity
• Constraining non standard recombination: A worked example
• Type Ia Supernovae and Cosmology
• Three problems about multi-scale modelling in cosmology
• A solution to the anisotropy problem in bouncing cosmologies
• Testing the DGP model with ESSENCE
• The variation of the gravitational constant inferred from the Hubble diagram of Type Ia supernovae
• Blind component separation in wavelet space. Application to CMB analysis
• Observational Constraints on Cardassian Expansion
• Natural Inflation, Planck Scale Physics and Oscillating Primordial Spectrum
• Stable and self consistent charged gravastar model within the framework of $f(R,T)$ gravity
• Dynamical effects of the scale invariance of the empty space: The fall of dark matter ?
• Second-order perturbations of cosmological fluids: Relativistic effects of pressure, multi-component, curvature, and rotation
• All-sky convolution for polarimetry experiments
• $f(R)$ gravity theories in the Palatini Formalism constrained from strong lensing
• The Cosmic Microwave Background for a Nearly Flat Compact Hyperbolic Universe
• Toward a Unified Description of Dark Energy and Dark Matter from the Abnormally Weighting Energy Hypothesis
• Two viable quintessence models of the Universe: confrontation of theoretical predictions with observational data
• Search for dark matter in proton-proton collisions at 8 TeV with missing transverse momentum and vector boson tagged jets
• Cosmological Density and Power Spectrum from Peculiar Velocities: Nonlinear Corrections and PCA
• On the Initial Conditions for Brane Inflation
• B-Pol: Detecting Primordial Gravitational Waves Generated During Inflation
• Chaos in the motion of a test scalar particle coupling to Einstein tensor in Schwarzschild-Melvin black hole spacetime
• Brane World Cosmologies with Varying Speed of Light
• Thermodynamics of interacting entropy-corrected holographic dark energy in a non-flat FRW universe
• Quintessence in a Brane World
• The generalized second law of gravitational thermodynamics on the apparent horizon in f(R)-gravity
• Using a phenomenological model to test the coincidence problem of dark energy
• A strategy for finding gravitationally-lensed distant supernovae
• The Integrated Sachs-Wolfe Effect in Interacting Dark Energy Models
• Holographic dark energy in Gauss-Bonnet gravity with Granda-Oliveros cut-off
• String inspired explanation for the super-acceleration of our universe
• Distance-Redshift in Inhomogeneous $Omeg{a}_0=1$ Friedmann-Lemaitre-Robertson-Walker Cosmology
• Detecting WIMPs in the Microwave Sky
• What the small angle CMB really tells us about the curvature of the Universe
• Implications for quintessence models from MAXIMA-1 and BOOMERANG-98
• Electromagnetic wave collapse in a radiation background
• Dynamics of Cosmological Perturbations in Position Space
• Unified Model for Dark Energy
• Probing the power spectrum bend with recent CMB data
• (1+3) Covariant Dynamics of Scalar Perturbations in Braneworlds
• Current and future supernova constraints on decaying $\Lambda$ cosmologies
• Supersymmetric topological inflation model
• Natural Quintessence with Gauge Coupling Unification
• Stability of FRW Cosmology with Generalized Chaplygin Gas
• $\gamma$ Parameter and Solar System constraint in Chameleon Brans Dick Theory
• Probing Noncommutativity with Inflationary Gravitational Waves
• Cosmological tests of the osculating Barthel-Kropina dark energy model
• Holography and the large number hypothesis
• How old is the Universe ? Setting new constraints on the age of the Universe
• A Cosmic Microwave Background Radiation Polarimeter Using Superconducting Bearings
• On the Formation of Degenerate Heavy Neutrino Stars
• Inflation and Braneworlds: Degeneracies and Consistencies
• Holographic dark energy in a non-flat universe with Granda-Oliveros cut-off
• QCD ghost f(T)-gravity model
• Position-Space Description of the Cosmic Microwave Background and Its Temperature Correlation Function
• Boomerang returns unexpectedly
• The Homogeneous Scalar Field and the Wet Dark Sides of the Universe
• Analysis of cosmic microwave background data on an incomplete sky
• Determining the equation of state of dark energy from angular size of compact radio sources and X-ray gas mass fraction of galaxy clusters
• Are Clusters Standard Candles? Galaxy Cluster Scaling Relations With the Sunyaev-Zeldovich Effect
• Genus Topology of the Cosmic Microwave Background from WMAP
• Weak lensing signal in Unified Dark Matter models
• Tight Cosmological Constraints from the Angular-Size/Redshift Relation for Ultra-Compact Radio Sources
• Confronting pNGB quintessence with data
• Modelling the Milky Way through adiabatic compression of cold dark matter halo
• Quintessence Unification Models from Non-Abelian Gauge Dynamics
• Extended Born-Infeld Dynamics and Cosmology
• Precision Cosmology and the Density of Baryons in the Universe
• The BOOMERANG North America Instrument: a balloon-borne bolometric radiometer optimized for measurements of cosmic background radiation anisotropies from 0.3 to 4 degrees
• Quintessence Restrictions on Negative Power and Condensate Potentials
• A dynamical stabilization of the radion potential
• Model Independent Primordial Power Spectrum from Maxima, Boomerang, and DASI Data
• Acoustic peaks and dips in the CMB power spectrum: observational data and cosmological constraints
• Inhomogeneous Big Bang Nucleosynthesis: Upper Limit on Omega_b and Production of Lithium, Beryllium, and Boron
• The 2dF QSO Redshift Survey - VII. Constraining Cosmology from Redshift Space Distortions via xi(sigma,pi)
• The Large-Scale Structure of the X-ray Background and its Cosmological Implications
• Cosmic (super)string constraints from 21 cm radiation
• Effects of quintessence on observations of Type Ia SuperNovae in the clumpy Universe
• Cosmic acceleration as the solution to the cosmological constant problem
• Neutrino flavor ratios as diagnostic of solar WIMP annihilation
• Dark energy and accelerating cosmological evolution from osculating Barthel-Kropina geometry
• Limits on the evolution of galaxies from the statistics of gravitational lenses
• Neutrino Oscillations, Lorentz/CPT Violation, and Dark Energy
• Transit cosmological models with observational constraints in f(Q, T) gravity
• A Preliminary Detection of Arcminute Scale Cosmic Microwave Background Anisotropy with the BIMA Array
• Dynamics and properties of chiral cosmic strings in Minkowski space
• Can brane cosmology with a vanishing Λexplain the observations?
• Effects of f(R) Dark Energy on Dissipative Anisotropic Collapsing Fluid
• Legacy data and cosmological constraints from the angular-size/redshift relation for ultra-compact radio sources
• Inflationary NonGaussianity from Thermal Fluctuations
• The angular power spectra of polarized Galactic synchrotron
• Constraints on Neutrino Degeneracy from the Cosmic Microwave Background and Primordial Nucleosynthesis
• Measuring the Chaplygin gas equation of state from angular and luminosity distances
• The angular power spectrum of radio emission at 2.3 GHz
• Cosmic Inflation at the Crossroads
• Dark Matter and Dark Energy from a single scalar field and CMB data
• From Anisotropy to Omega
• Distances in inhomogeneous quintessence cosmology
• CMB Bispectrum from Active Models of Structure Formation
• de Sitter Relativity: a New Road to Quantum Gravity?
• Constraints on the Cosmological Relativistic Energy Density
• The morphological and dynamical evolution of simulated galaxy clusters
• Exact solutions in bouncing cosmology
• Cosmic Microwave Background Anisotropy with Cosine-Type Quintessence
• Fluctuations in the CMB Induced by Cosmic Strings: Methods and Formalism
• A Non-minimally Coupled Quintom Dark Energy Model on the Warped DGP Brane
• Polytropic dark matter flows illuminate dark energy and accelerated expansion
• Scale Factor Dependent Equations of State for Curvature Inspired Dark Energy, Phantom Barrier and Late Cosmic Acceleration
• Marginally Stable Circular Orbits in Schwarzschild Black Hole Surrounded by Quintessence Matter
• Universal thermodynamics in different gravity theories: Modified entropy on the horizons
• The ROSAT-ESO Flux-Limited X-Ray (REFLEX) Galaxy Cluster Survey VI: Constraints on the cosmic matter density from the KL power spectrum
• Brane inflation driven by noncanonical scalar field
• Rethinking Lensing and Lambda
• Holographic, new agegraphic and ghost dark energy models in fractal cosmology
• Wormhole on the Brane with Ordinary Matter: The Broader View
• Cosmic Microwave Background Acoustic Peak Locations
• Weighing the Universe with Photometric Redshift Surveys and the Impact on Dark Energy Forecasts
• Extended quintessence, inflation, and stable de Sitter spaces
• Addendum to: Update on neutrino mixing in the early Universe
• Accelerating Bianchi Type-V Cosmology with Perfect Fluid and Heat Flow in Saez-Ballester Theory
• Nonlinear electrodynamics in Bianchi spacetimes
• Frequentist Estimation of Cosmological Parameters from the MAXIMA-1 Cosmic Microwave Background Anisotropy Data
• Beam mismatch effects in Cosmic Microwave Background polarization measurements
• Gravitationally induced particle production in scalar-tensor $f(R,T)$ gravity
• Constraints on self-interacting Q-ball dark matter
• The statistics of wide-separation lensed quasars
• Constraining our Universe with X-ray & Optical Cluster Data
• WMAP constraints on Cardassian model
• Is thermodynamics of the universe bounded by the event horizon a Bekenstein system?
• Cluster correlations in redshift space
• Apparent Clustering of Intermediate-redshift Galaxies as a Probe of Dark Energy
• Frame-independence of the Inhomogeneous Mixmaster Chaos via Misner-Chitre'-like variables
• Likelihood methods for CMB experiments
• Statefinder diagnosis for holographic dark energy in the DGP braneworld
• Quantum vacuum, dark matter, dark energy and spontaneous supersymmetry breaking
• The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity
• Collision-induced galaxy formation: semi-analytical model and multi-wavelength predictions
• Agegraphic Chaplygin gas model of dark energy
• PLANCK: systematic effects induced by periodic fluctuations of arbitrary shape
• Why Does Gravity Ignore the Vacuum Energy?
• Comparison between the Logotropic and $\Lambda$CDM models at the cosmological scale
• Squark-, Slepton- and Neutralino-Chargino coannihilation effects in the low-energy effective MSSM
• WMAPping out Neutrino Masses
• Constraints on extra dimensions from cosmological and terrestrial measurements
• Perturbative approach for mass varying neutrinos coupled to the dark sector in the generalized Chaplygin gas scenario
• Redshift-Space Enhancement of Line-of-Sight Baryon Acoustic Oscillations in the SDSS Main-Galaxy Sample
• A redefinition of Hawking temperature on the event horizon: Thermodynamical equilibrium
• Constraints on alternative models to dark energy
• Density Fluctuations and Primordial Black Hole Formation in Natural Double Inflation in Supergravity
• Planck LFI: Comparison Between Galaxy Straylight Contamination and other Systematic Effects
• Reconstructing interacting new agegraphic polytropic gas model in non-flat FRW universe
• Cosmic acceleration in non-canonical scalar field model - An interacting scenario
• The Polarization of the Cosmic Microwave Background Due to Primordial Gravitational Waves
• Cluster Morphologies as a Test of Different Cosmological Models
• Anisotropic cosmologies containing isotropic background radiation
• A Stochastic Measure for Eternal Inflation
• Future Evolution of the Intergalactic Medium in a Universe Dominated by a Cosmological Constant
• Stability of accelerating cosmology in two scalar-tensor theory: Little Rip versus de Sitter
• Probing large-distance higher-dimensional gravity with Cosmic Microwave Background measurements
• Galaxy surveys, inhomogeneous reionization, and dark energy
• Searching For Dark Matter with Neutrino Telescopes
• The Sky Polarization Observatory
• How Recent is Cosmic Acceleration?
• Non-chaotic dynamics in general-relativistic and scalar-tensor cosmology
• The 2dF QSO Redshift Survey - IV. The QSO Power Spectrum from the 10k Catalogue
• Two-point correlation functions on the light cone: testing theoretical predictions against N-body simulations
• Constraints on scalar and tensor perturbations in phenomenological and two-field inflation models: Bayesian evidences for primordial isocurvature and tensor modes
• New exact solutions for inflationary cosmological perturbations
• Constraints on the non-linear coupling parameter fnl with the Archeops data
• CMB anisotropy science: a review
• The Core-Cusp Problem Revisited: ULDM vs. CDM
• BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data
• Active-Sterile neutrino oscillations and BBN+CMBR constraints
• Quasinormal modes of black holes absorbing dark energy
• Cosmic strings, loops, and linear growth of matter perturbations
• Non-Gaussianity, Isocurvature Perturbation, Gravitational Waves and a No-Go Theorem for Isocurvaton
• Observational evidence for a correlation between peak-luminosities and beaming in GRBs
• Late-time acceleration and Phantom Divide Line Crossing with Non-minimal Coupling and Lorentz Invariance Violation
• Holographic Dark Energy from a Modified GBIG Scenario
• Particle decay in the early universe: predictions for 21 cm
• Effect of quintessence on the energy of the Reissner-Nordstrom black hole
• Scalar-field theory of dark matter
• Interacting Two-Fluid Viscous Dark Energy Models In Non-Flat Universe
• Some new class of Chaplygin Wormholes
• A Cyclic Universe With Varying Cosmological Constant in $f(R,T)$ gravity
• SN1A data and the CMB of Modified Curvature at short and long distances
• Limits on the Detectability of Cosmic Topology in Hyperbolic Universes
• Arbitrary Dimensional Schwarzschild-FRW Black Holes
• New self-consistent effective one-body theory for spinless binaries based on the post-Minkowskian approximation
• Infinity in string cosmology: A review through open problems
• Quintessence with two energy scales
• Evidence for a Significant Blazar Contamination in CMB Anisotropy Maps
• Conceptual Problems of Inflationary Cosmology and a New Approach to Cosmological Structure Formation
• SNLS data are consistent with acceleration at z=3
• Early and Late Transient Cosmic Acceleration due to Curvature Inspired Dark Energy
• Lagrangian evolution of global strings
• Slow-roll inflation and CMB anisotropy data
• Stable accelerating universe with no hair
• A Dynamical Study of the Friedmann Equations
• Two-Fluid Dark Energy Models in Bianchi Type-III Universe with Variable Deceleration Parameter
• Polarization observations in a low synchrotron emission field at 1.4 GHz
• Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension
• Dark energy models toward observational tests and data
• Full-sky correlations of peaks in the microwave background
• Geometrical estimators as a test of Gaussianity in the CMB
• The Influence of Free Quintessence on Gravitational Frequency Shift and Deflection of Light with 4D momentum
• Self-consistent Effective-one-body theory for spinless binaries based on post-Minkowskian approximation I: Hamiltonian and decoupled equation for ${\psi }_4^B$
• The flavor vacuum in the expanding universe and dark matter
• Holographic kinetic k-essence model
• Harmonic analysis of cosmic microwave background data II: from ring-sets to the sky
• A Braneworld Dark Energy Model with Induced Gravity and the Gauss-Bonnet Effect
• The Cosmic Baryon Fraction and the Extragalactic Ionizing Background
• A Specific Case of Generalized Einstein-aether Theories
• Probing modified gravity theories with the Sandage-Loeb test
• The generalized second law for the interacting generalized Chaplygin gas model
• CMB Constraints on a Baryonic Dark Matter-Dominated Universe
• Model-independent study for a quintessence model of dark energy: Analysis and Observational constraints
• Fitting BOOMERANG and MAXIMA-1 data with a Einstein-Yang-Mills Cosmological Model
• Rotation Curves of Galaxies by Fourth Order Gravity
• FRW Cosmology From Five Dimensional Vacuum Brans-Dicke Theory
• Observational constraints on the spectral index of the cosmological curvature perturbation
• Limits on Cosmic Matter--Antimatter Domains from Big Bang Nucleosynthesis
• Thermodynamical description of the interacting new agegraphic dark energy
• CMB power spectrum estimation using noncircular beams
• Interacting entropy-corrected new agegraphic dark energy in non-flat universe
• Galaxy Bias in Quintessence Cosmological Models
• Physics of the cosmic microwave background anisotropy
• Elliptic CMB Sky
• A small universe after all?
• Determining the Geometry and the Cosmological Parameters of the Universe through SZE Cluster Counts
• How is the Reionization Epoch Defined?
• Interacting New Agegraphic Dark Energy in a Cyclic Universe
• Equation of state of cosmic strings with fermionic current-carriers
• Limits on decaying dark energy density models from the CMB temperature-redshift relation
• Cosmography and large scale structure by f(R) gravity: new results
• Cosmic magnetic fields from velocity perturbations in the early Universe
• Vacuum Energy as the Origin of the Gravitational Constant
• A conventional approach to the dark-energy concept
• Palatini formulation of modified gravity with squared scalar curvature
• Boson mixing and flavor vacuum in the expanding Universe: a possible candidate for the dark energy
• Unification of the first law of quantum thermodynamics
• Dark Energy: The Shadowy Reflection of Dark Matter?
• Ionization history of the Universe as a test for Super Heavy Dark Matter particles
• Testing the (generalized) Chaplygin gas model with the Lookback time-Redshift data
• Comparison of Frames: Jordan vs Einstein Frame for a Non-minimal Dark Energy Model
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• Non-Newtonian Gravity, Fluctuative Hypothesis and the Sizes of Astrophysical Structures
• Cosmological anisotropy from non-comoving dark matter and dark energy
• New Constraints on the Variable Equation of State Parameter from X-Ray Gas Mass Fractions and SNe Ia
• Curvature Inspired Cosmological Scenario
• Role of Modified Chaplygin Gas as a Dark Energy Model in Collapsing Spherically Symmetric Cloud
• A fluid os strings as a viable candidate to the dark side of the universe
• Anisotropic solid dark energy
• Running vacuum in Brans-Dicke theory: a possible cure for the ${\sigma }_8$ and $H_0$ tensions
• Uniqueness of the Fock quantization of scalar fields under mode preserving canonical transformations varying in time
• Cosmological Evolution of Global Monopoles
• Brane-Bulk energy exchange and agegraphic dark energy
• Limits Due to Instrumental Polarisation in CMB Experiments at Microwave Wavelengths
• Crossing of the Phantom Divided Barrier with Lorentz Invariance Violating Fields
• Decaying neutrino and a high cosmological baryon density
• Irreversibility of Time for Quasi-Isolated Systems
• Acceleressence: Dark Energy from a Phase Transition at the Seesaw Scale
• The spectral action and cosmic topology
• Brans-Dicke Cosmology in 4D from scalar-vacuum in 5D
• Analytic solutions for the $\Lambda$-FRW Model
• BOOMERanG Constraints on Primordial Non-Gaussianity from Analytical Minkowski Functionals
• Possible flakes of molecular hydrogen in the early Universe
• Holographic dark energy with the sign-changeable interaction term
• Constraint on Cosmological Model with Matter Creation Using Complementary Astronomical Observations
• Global fits for the spectral index of the cosmological curvature perturbation
• Cosmological Parameters from Redshift-Space Correlations
• Fermionic massive modes along cosmic strings
• Cosmological evolution of interacting dark energy in Lorentz violation
• Brane-Universes with Variable G and Lambda
• The 2dF QSO Redshift Survey - VI. Measuring Lambda and Beta from Redshift-space Distortions in the Power Spectrum
• Higher neutrino mass allowed if Cold Dark Matter and Dark Energy are coupled
• Rip/singularity free cosmology models with bulk viscosity
• Accelerating Universe in a Big Bounce Model
• Group theoretical interpretation of the modified gravity in de Sitter space
• Dark energy interacting with dark matter and unparticle
• Late reionizations of the Universe and their manifestation in the CMB data
• Age of the Universe in the Cardassian Model
• A Singular Conformal Spacetime
• Corrected holographic dark energy with power-law entropy and Hubble Horizon cut-off in FRW Universe
• On the Stewart-Lyth Inverse Problem
• An exact model of conformal quintessence
• The nature of $\Lambda$ and the mass of the graviton: A critical view
• The tight-coupling approximation for baryon acoustic oscillations
• Constraints on the Cardassian Expansion from the Cosmic Lens All-Sky Survey Gravitational Lens Statistics
• Constraints on the cosmic equation of state: age conflict versus phantom energy. Age-redshift relations in an accelerated universe
• Using the COBE/DMR data as a test-bed for normality assessments
• Acceleration of the Universe
• Potential--density pairs for spherical galaxies and bulges: the influence of scalar fields
• Surface vacuum energy and stresses for a brane in de Sitter spacetime
• Friedmann Equation for Brans Dicke Cosmology
• Partial rip scenario - a cosmology with a growing cosmological term
• Sounds of instability from generalized QCD ghost dark energy
• Gödel-type solutions within the f(R,Q) gravity
• Ellipticity in Cosmic Microwave Background as a Tracer of Large-Scale Universe
• MAXIMA: A Balloon-Borne Cosmic Microwave Background Anisotropy Experiment
• Strong gravitational lensing by a Konoplya-Zhidenko rotating non-Kerr compact object
• Stewart-Lyth Inverse Problem
• Tension between SN and BAO: current status and future forecasts
• Inflessence: a phenomenological model for inflationary quintessence
• Thermodynamical description of the ghost dark energy model
• Anisotropic $k$-essence
• Reconstruction of $f(R,T)$ gravity model via the Raychaudhuri equation
• Bayesian joint estimation of non-Gaussianity and the power spectrum
• Quantum Theory on Lobatchevski Spaces
• Tomography from the Next Generation of Cosmic Shear Experiments for Viable f(R) Models
• A stable flat universe with variable Cosmological constant in f(R,T) Gravity
• The power spectrum of galaxy clustering in the APM survey
• Interacting Tsallis and Rényi Holographic Dark Energy with Hybrid Expansion Law
• A tensor theory of space-time as a strained material continuum
• Reheating and dangerous relics in pre-big bang string cosmology
• New Concept for Testing General Relativity: The Laser Astrometric Test of Relativity (LATOR) Mission
• Cosmological Black Holes as Seeds of Voids in Galaxy Distribution
• BeyondPlanck VII. Bayesian estimation of gain and absolute calibration for CMB experiments
• Mirage: a new iterative Map-Making code for CMB experiments
• Current constraints on Cosmological Parameters from Microwave Background Anisotropies
• Gravitationally induced matter creation in scalar-tensor $f(R,T_{\mu \nu }{T}^{\mu \nu })$ gravity
• Measuring ${\sigma }_8$ using DESI Legacy Imaging Surveys Emission-Line Galaxies and Planck CMB Lensing and the Impact of Dust on Parameter Inference
• Constraints on Omega_B, Omega_m and h from MAXIMA and BOOMERANG
• Testing the local void hypothesis using baryon acoustic oscillation measurements over the last twenty years
• Large Scale Plane-Mirroring in the Cosmic Microwave Background WMAP5 Maps
• Subaru Spectroscopy of the Gravitational Lens HST 14176+5226: Implications for a Large Cosmological Constan
• Deflationary $\Lambda (t)$ cosmology: observational expressions
• Constraints on Quintessence From Using Cosmological Data
• Quintessential brane cosmology
• Einstein's Biggest Blunder? High-Redshift Supernovae and the Accelerating Universe
• Luminosity Function of GRBs
• Blind component separation for polarized observations of the CMB
• Constraining the Cosmological Constant from Large-Scale Redshift-Space Clustering
• Charged gravastar model in Rastall theory of gravity
• Anisotropic bulk viscous string cosmological models of the Universe under a time-dependent deceleration parameter
• Constraints from the CMB temperature and other common observational data-sets on variable dark energy density models
• Dark Energy and the Hubble Age
• Comparing and combining the Saskatoon, QMAP and COBE CMB maps
• Matching torsion Lambda - term with observations
• Transverse Wave Propagation in Relativistic Two-fluid Plasmas around Schwarzschild-de Sitter Black Hole
• Inhomogeneous Big Bang Nucleosynthesis and the High Baryon Density Suggested by Boomerang and MAXIMA
• N = 2 Supersymmetry in a Hybrid Inflation Model
• Implications of the WMAP Age Measurement for Stellar Evolution and Dark Energy
• The coupling of topology and inflation in Noncommutative Cosmology
• Dark Energy: The Observational Challenge
• Casimir energy-momentum tensor for the Robin Surfaces in de Sitter Spacetime
• Reconstructing the properties of dark energy from recent observations
• Observational constraints on the interacting dark energy - dark matter (IDM) cosmological models
• Small Second Acoustic Peak from Interacting Cold Dark Matter?
• Scaling property and peculiar velocity of global monopoles
• Peaks in the CMBR power spectrum. II. Physical interpretation for any cosmological scenario
• Modified Dark Matter: Relating Dark Energy, Dark Matter and Baryonic Matter
• Tracing the Nature of Dark Energy with Galaxy Distribution
• A Complete Cosmological Scenario in Teleparallel Gravity
• Bumpy Power Spectra and dT/T
• Gravitational Lensing Constraints on Dynamical and Coupled Dark Energy
• Dark matter and dark energy induced by condensates
• Effective cosmological "constant " and quintessence
• RHDE models in FRW Universe with two IR cut-offs with redshift parametrization
• BeyondPlanck XII. Cosmological parameter constraints with end-to-end error propagation
• A Two-field Dilaton Model of Dark Energy
• The CMB power spectrum at l=30-200 from QMASK
• Weak Gravitational Lensing in Fourth Order Gravity
• Supernovae as a probe of particle physics and cosmology
• Detectability of Cosmic Topology in Flat Universes
• Residual noise covariance for Planck low-resolution data analysis
• CMB anisotropies from pre-big bang cosmology
• The Central Mass and Phase-Space Densities of Dark Matter Halos: Cosmological Implications
• The New Cosmology
• A heuristic wave equation parameterizing BEC dark matter halos with a quantum core and an isothermal atmosphere
• A measurement at the first acoustic peak of the CMB with the 33 GHz interferometer
• Kaluza-Klein Type Robertson Walker Cosmological Model With Dynamical Cosmological Term $\Lambda$
• Cosmological Black Holes
• Reproducing the observed Cosmic microwave background anisotropies with causal scaling seeds
• Small-Scale Cosmic Microwave Background Polarization from Reionization
• Leptogenesis in a Realistic Supersymmetric Model of Inflation with a Low Reheat Temperature
• Curvature Dependence of Peaks in the Cosmic Microwave Background Distribution
• Optimized in-flight absolute calibration for extended CMB surveys
• Thermodynamic of universe with a varying dark energy component
• The Angular Power Spectrum of the First-Year WMAP Data Reanalysed
• The primordial baryonic clouds and their contribution to the CMB anisotropy and polarization formation
• Scalar Field Dark Matter
• Brane World Linearized Cosmic String Gravity
• Neutrino Dark Energy and Moduli Stabilization in a BPS Braneworld Scenario
• Influences of Dark Energy and dark matter on Gravitational Time Advancement
• Phantom Cosmology with Non-minimally Coupled Real Scalar Field
• Uncertainty on determining the dark energy equation of state due to the spatial curvature
• On Bianchi type III Cosmological Model with Quadratic EoS in Lyra Geometry
• Interacting Holographic Dark Energy, the Present Accelerated Expansion and Black Holes
• POKER: Estimating the power spectrum of diffuse emission with complex masks and at high angular resolution
• The lepton asymmetry: the last chance for a critical-density cosmology?
• An extended analysis for a generalized Chaplygin gas model
• Dark Energy From Fifth Dimensional Brans-Dicke Theory
• Interacting entropy-corrected holographic Chaplygin gas model
• Do recent observations favor a cosmological event horizon: A thermodynamical prescription?
• On the spacetime connecting two aeons in conformal cyclic cosmology
• Future Island Universes in a Background Universe Accelerated by Cosmological Constant and by Quintessence
• Cosmological parameters from complementary observations of the Universe
• Scalar field-perfect fluid correspondence and nonlinear perturbation equations
• Testing and selection of cosmological models with $(1+z{)}^6$ corrections
• The 60-micron extragalactic background radiation intensity, dust-enshrouded AGNs and the assembly of groups and clusters of galaxies
• The generalized second law for the interacting new agegraphic dark energy in a non-flat FRW universe enclosed by the apparent horizon
• Interacting agegraphic quintessence dark energy in non-flat universe
• Concerning Parameter Estimation Using the Cosmic Microwave Background
• The cosmological evolution of colour gradients in spheroids
• Late time cosmic acceleration from vacuum Brans-Dicke theory in 5D
• Holographic dark energy interacting with dark matter in a Closed Universe
• FLRW accelerating universe with interactive dark energy
• Dynamical-Screening and the Phantom-Like Effects in a DGP-Inspired $F(R,\varphi )$ Model
• Direct Search for Dark Matter - Striking the Balance - and the Future
• Testing Dark Energy with the Advanced Liquid-Mirror Probe of Asteroids, Cosmology and Astrophysics
• Statefinder parameters for quantum effective Yang-Mills condensate dark energy model
• Is Noncommutative Eternal Inflation Possible?
• A Sober Assessment of Cosmology at the New Millennium
• Bounding $f(R)$ gravity by particle production rate
• Fast Parameter Estimation from the CMB Power Spectrum
• Dark Energy Nature in Logarithmic $f(R,T)$ Cosmology
• A Dark Energy Quintessence Model of the Universe
• On Dark Energy and Accelerated Reference Frames
• Flat Universe with Hyperbolic Voids
• An FLRW interacting dark energy model of the Universe
• Ricci Dark Energy of Amended FRW Universe in Chern-Simon Modified Gravity
• Interacting Viscous Dark Energy in Bianchi Type-I Universe
• The mass function of the Las Campanas loose groups of galaxies
• A Direct Upper Limit on the Density of Cosmological Dust from the Absence of an X-ray Scattering Halo around the z=4.3 QSO 1508+5714
• Ellipticity analysis of the BOOMERanG CMB maps
• Potential-density pairs for axisymmetric galaxies: the influence of scalar fields
• Using machine learning to compress the matter transfer function $T(k)$
• Quantum driven Bounce of the future Universe
• Gravitational Collapse in Higher Dimensional Husain Space-Time
• Tests of AMiBA Data Integrity
• Knotlike Cosmic Strings in The Early Universe
• Reconstruction of $5D$ Cosmological Models From Equation of State of Dark Energy
• Generalized Self-similar Scalar-Tensor Theories
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• Observations of the High Redshift Universe
• Map-making methods for Cosmic Microwave Background experiments
• Testing Gaussianity on Archeops Data
• Correlations Between the WMAP and MAXIMA Cosmic Microwave Background Anisotropy Maps
• Non-linear Preheating with Scalar Metric Perturbations
• Scale Invariance, Horizons, and Inflation
• Determining Foreground Contamination in CMB Observations: Diffuse Galactic Emission in the MAXIMA-I Field
• Graviton mass and total relative density of mass Omega_tot in Universe
• Self-Dual Cosmic Strings and Gravitating Vortices in Gauged Sigma Models
• Thermodynamic behavior and stability of Polytropic gas
• Clusters of galaxies: setting the stage
• Slepton and Neutralino/Chargino Coannihilations in MSSM
• Cosmology from Cosmic Microwave Background and Galaxy Clusters
• Quintessence Model and Observational Constraints
• Primordial and asymptotic inflation in Brans-Dicke cosmology
• A flat FRW model with dynamical $\Lambda$ as function of matter and geometry
• The History of Astrophysics in Antarctica
• Correlation of the South Pole 94 data with 100microns and 408 MHz maps
• Phantom Accretion by Black Holes and the Generalized Second Law of Thermodynamics
• FRW dark energy cosmological model with hybrid expansion law
• Why Are Neutrinos Light? -- An Alternative
• Whether Lyra's Manifold Itself is a Hidden Source of Dark Energy
• Dynamical Dark Energy model parameters with or without massive neutrinos
• Relic gravitational waves and the generalized second law
• Modular thermal inflation without slow-roll approximation
• Universal thermodynamics in different gravity theories: Conditions for generalized second law of thermodynamics and thermodynamical equilibrium on the horizons
• Needatool: A Needlet Analysis Tool for Cosmological Data Processing
• Omega_m - Different Ways to Determine the Matter Density of the Universe
• Systematics in the Gamma Ray Bursts Hubble diagram
• The nature of the red disk-like galaxies at high redshift: dust attenuation and intrinsically red stellar populations
• Using the acoustic peak to measure cosmological parameters
• Vacuum Bubbles Nucleation and Dark Matter Production through Gauge Symmetry Rearrangement
• Constraints on Natural Inflation from Cosmic Microwave Background
• A Study of Universal Thermodynamics in Brane World Scenario
• Energy extraction from a Konoplya-Zhidenko rotating non-Kerr black hole
• COSMOSOMAS: A Circular Scanning Instrument to Map the Sky at Centimetric Wavelengths
• Interaction between phantom field and modified Chaplygin gas
• Consistency of nonlinear interacting ghost dark energy with recent observations
• Astrophysical structures from primordial quantum black holes
• Axial Anomaly in Galaxies and the Dark Universe
• Subdegree Sunyaev-Zel'dovich Signal from Multifrequency BOOMERanG observations
• 'Steckbrief' Lambda
• Constraining Cosmological Models by the Cluster Mass Function
• Thermal fluctuations in viscous cosmology
• Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys
• First-order perturbations of Gödel-type metrics in non-dynamical Chern-Simons modified gravity
• Is Physics Asking for a New Kinematics?
• The link between E-B polarization modes and gas column density from interstellar dust emission
• Interacting generalized ghost dark energy in non-flat universe
• Determining cosmic microwave background structure from its peak distribution
• Galaxy-QSO Correlation induced by Weak Gravitational Lensing arising from Large-Scale Structure
• Super-gauge Field in de Sitter Universe
• Chameleonic dilaton, nonequivalent frames, and the cosmological constant problem in quantum string theory
• SU(2)${}_{\mathrm{CMB}}$ and the cosmological model: angular power spectra
• Study of QCD generalized ghost dark energy in FRW universe
• Cosmological simulations using a static scalar-tensor theory
• Constraints from the damping tail
• On Axial and Plane--Mirror Inhomogeneities in the WMAP3 Cosmic Microwave Background Maps
• Newtonian limit of String-Dilaton Gravity
• Search for dark matter particles in proton-proton collisions at sqrt(s) = 8 TeV using the razor variables
• SNe Ia Tests of Quintessence Tracker Cosmology in an Anisotropic Background
• Recent Results from the MAXIMA Experiment
• Holographic dilatonic model of dark energy
• On the luminosity distance and the epoch of acceleration
• Irreversible thermodynamics of dark energy on entropy-corrected apparent horizon
• F(R) cosmology via Noether symmetry and lambda-Chaplygin Gas like model
• Quantum gravitational signatures in next-generation gravitational wave detectors
• Simultaneous determination of ${\Omega }_{M0}$ and $H_0$ from joint Sunyaev-Zeldovich effect and X-ray observations with median statistics
• Interacting Ricci Logarithmic Entropy Corrected Holographic Dark Energy in Brans-Dicke Cosmology
• Cosmological models of generalized ghost pilgrim dark energy (GGPDE) in the gravitation theory of Saez-Ballester
• Testing Unification and Dark Matter with Gravitational Waves
• From nuclei to atoms and molecules: the chemical history of the early Universe
• The supercluster-void network V. Alternative evidence for its regularity
• UHECR as Decay Products of Heavy Relics? The Lifetime Problem
• Stable phantom-divide crossing in two scalar models with matter
• Warm inflation with non-comoving scalar field and radiation fluid
• Probing the dark energy with quasar clustering
• Broadband anti-reflective coatings for cosmic microwave background experiments
• Transition from decelerated to accelerated cosmic expansion in braneworld universes
• Dissipative quintessence, and its cosmological implications
• Properties of the Top Quark
• On primordial trispectrum from exchanging scalar modes in general multiple field inflationary models
• A new asymptotical flat and spherically symmetric solution in the generalized Einstein-Cartan-Kibble-Sciama gravity and gravitational lensing
• Numerical computation of Maass waveforms and an application to cosmology
• Relationship between Bondi-Sachs quantities and source of gravitational radiation in asymptotically de Sitter spacetime
• Weak gravitational lensing by compact objects in fourth order gravity
• The Farthest Known Supernova: Support for an Accelerating Universe and a Glimpse of the Epoch of Deceleration
• Suppression of Gravitational Structure Formation by Cosmological Accretion Heating
• Cosmological constraints on dark energy
• Structure and evolution of Zel'dovich pancakes as probes of dark energy models
• Predictions of mixed non-Gaussian cosmological density fields for the cosmic microwave background radiation
• Particle Creation in Pre-Big-Bang Cosmology: theory and observational consequences
• Quantum Statistical Entropy and Minimal Length of 5D Ricci-flat Black String with Generalized Uncertainty Principle
• Detectability of Gravitational Lensing Effect on the Two-point Correlation Function of Hotspots in the CMB maps
• Interacting viscous entropy-corrected holographic scalar field models of dark energy with time-varying G in modified FRW cosmology
• Summary of Neutrino 2000
• No evidence for EDE from Planck data in extended scenarios
• Constraints on Cardassian universe from Gamma ray bursts
• Local Constraints on the Oscillating G Model
• Thermal non-Gaussianity in holographic cosmology
• A Comparison of Quintessence and Nonlinear Born-Infeld Scalar Field Using Gold Supernova data
• WMAP Constraints on Quintessence
• Reionization Constraints on the Contribution of Primordial Compact Objects to Dark Matter
• Interacting holographic tachyon model of dark energy
• Quintessence and variation of the fine structure constant in the CMBR
• The Logotropic Dark Fluid: Observational and Thermodynamic Constraints
• Asymmetric Dark Matter from Gravitational Waves
• Testing the ABS method with the simulated Planck temperature maps
• Observable interactions of quintessence with ordinary matter and neutrinos
• Ghost dark energy with sign-changeable interaction term
• Spectral Indications of thermal Sunyaev-Zel'dovich Effect in Archeops and WMAP Data
• Shortcuts in Domain Walls and the Horizon Problem
• Rapid onset of the 21-cm signal suggests a preferred mass range for dark matter particle
• On the primordial helium content: CMB and stellar constraints
• Mixed fluid cosmological model in $f(R,T)$ gravity
• On the coupling between different species during recombination
• Amplitude-Phase Analysis of Cosmic Microwave Background maps
• Testing feasibility of scalar-tensor gravity by scale dependent mass and coupling to matter
• Recent CMB Observations and the Ionization History of the Universe
• Thermodynamic descriptions of Polytropic gas and its viscous type as the dark energy candidates
• Black hole entropy arising from massless scalar field with Lorentz violation induced by the coupling to Einstein tensor
• Viscous Dark Energy and Phantom Field in An Anisotropic Universe
• Scale-Free model for governing universe dynamics
• Machine learning unveils the linear matter power spectrum of modified gravity
• Gravitational lensing constraint on the cosmic equation of state
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• Exact solution to perturbative conformal cosmology in the recombination era
• Topology of the Las Campanas Redshift Survey
• CMB Telescopes and Optical Systems
• Gödel-type solutions within the $f(R,Q,P)$ gravity
• Analytical solutions of the geodesic equation in the space-time of a black hole surrounded by perfect fluid in Rastall theory
• A weakly random Universe?
• Accelerating Cosmic Microwave Background map-making procedure through preconditioning
• Higher-order gravity in higher dimensions: Geometrical origins of four-dimensional cosmology?
• Scalar Field as Dark Energy Accelerating Expansion of the Universe
• Discord in Concordance Cosmology and Anomalously Massive Early Galaxies
• Thermodynamic analysis of universes with the initial and final de-Sitter eras
• A Viable Dark Fluid Model
• Posing Constraints on the Free Parameters of a New Model of Dark Energy EoS : Responses Through Cosmological Behaviours
• Probing large-scale structure with large samples of X-ray selected AGN: I Baryonic acoustic oscillations
• A Theory of time-varying Constants
• Latest Observational Constraints on Cardassian Models
• Is there a common origin for the WMAP low multipole and for the ellipticity in BOOMERanG CMB maps?
• CMB Polarization as complementary information to anisotropies
• Closed universe and the first Doppler-peak of the CMB spectrum
• Two Dynamical Scenarios for Binned Master Sample Interpretation
• Probing departures from $\Lambda$CDM by late-time datasets
• Fundamental Approach to the Cosmological Constant Issue
• Stability analysis of an interacting holographic dark energy model
• Aspects of Some New Versions of Pilgrim Dark Energy in DGP Braneworld
• Nonlinear Behavior of Baryon Acoustic Oscillations in Redshift Space from the Zel'dovich Approximation
• Implications of the BOOMERANG and MAXIMA-I results for the Baryon Mass Fraction in Clusters of galaxies
• Inflationary scenarios with scale-invariant spectral tensorial index
• Asymptotic behaviour of cylindrical waves interacting with spinning strings
• Morphological Number Counts and Redshift Distributions to I = 25 from the Hubble Deep Fields: Constraints on Cosmological Models from Early Type Galaxies
• Voids and overdensities of coupled Dark Energy
• Non-singular inflation with vacuum decay
• Universe consisting of diffusive dark fluids: thermodynamics and stability analysis
• Tsallis holographic inflation in $f(R,T)$ gravity: CMB constraints, reheating, and swampland implications
• "Expansion" around the vacuum: how far can we go from Lambda?
• Relativistic corrections to fractal analyses of the galaxy distribution
• Validation of Emission-Line Galaxies Target Selection Algorithms for the Dark Energy Spectroscopic Instrument Using the MMT Binospec
• Effects on the structure of the universe of an accelerating expansion
• Lorentz violation with an invariant minimum speed as foundation of the uncertainty principle in Minkowski, dS and AdS spaces
• The shape of a small universe: signatures in the cosmic microwave background
• Dark matter annihilation and non-thermal Sunyaev-Zel'dovich effect: I. galaxy cluster
• Reconstruction of Five-dimensional Bounce cosmological Models From Deceleration Factor
• Cosmic ray threshold in an asymptotically dS spacetime
• Acceptable Inverse Power Law Potential Quintessence with n=18/7
• Theoretical Models of Multi-waveband QSO Luminosity Functions
• The exact analytical solution of the linear structure growth rate in LCDM cosmology and its cosmological applications
• What can be learned about dark energy evolution?
• How accurately can we measure the hydrogen 2S->1S transition rate from the cosmological data?
• Observational Matter Power Spectrum and the Height of the Second Acoustic Peak
• The Spectre of Underdetermination in Modern Cosmology
• Quintessential Inflation with Dissipative fluid
• Thermodynamical description of modified generalized Chaplygin gas model of dark energy
• Curvature of the universe and the dark energy potential
• Cosmic acceleration from second order gauge gravity
• Cosmic opacity to CMB photons and polarization measurements
• Controlling systematics in ground-based CMB surveys with partial boresight rotation
• Reconstructing the parameter space of non-analytical cosmological fixed points
• A proposal to improve the accuracy of cosmological observables and address the Hubble tension problem
• Cosmological models based on a complex scalar field with a power-law potential associated with a polytropic equation of state
• Cosmic String Signatures in the Cosmic Microwave Background Anisotropies
• Bouncing Universe with a Nonminimally Coupled Scalar Field on a Moving Domain Wall
• Detection of Iron Emission in the z = 5.74 QSO SDSSp J104433.04-012502.2
• Dark energy induced by neutrino mixing
• Separation of foreground and background signals in single frequency measurements of the CMB Polarization
• A brief review of a modified relativity that explains cosmological constant
• Crossing of the Cosmological Constant Boundary - an Equation of State Description
• Structure formation and CMBR anisotropy spectrum in the inflessence model
• Constraining the reionization history with large angle CMB polarization
• de Sitter invariant special relativity and galaxy rotation curves
• Global monopoles can change Universe's topology
• Linear perturbations in a universe with a cosmological constant
• An Interacting Scenario for Dark Energy in Bianchi Type-I Universe
• On the cosmological gravitational waves and cosmological distances
• Evolution of spherical over-densities in tachyon scalar field model
• Status and Perspectives of Neutrino Physics
• Can inflationary models of cosmic perturbations evade the secondary oscillation test?
• Correlation measurement of propagating microwave photons at millikelvin
• Implications to CMB from Model Independent evolution of w and Late Time Phase Transition
• Cosmological models with flat spatial geometry
• The effect of supersymmetry breaking in the Mass Varying Neutrinos
• Considering Late-Time Acceleration in some Cosmological Models
• Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
• Defect Formation Rates in Cosmological First-Order Phase Transitions
• Intermediate Scale Supersymmetric Inflation, Matter and Dark Energy
• Constraints on Brane-Localized Gravity
• Numerical Analysis of Galactic Rotation Curves
• A Dynamical Solution of Stable Starobinsky-Type Inflation Model in Quantum Geometry
• Pattern Universes
• Can Geometric Test Probe the Cosmic Equation of State ?
• Have Acoustic Oscillations been Detected in the Current Cosmic Microwave Background Data?
• Modeling dark energy through an Ising fluid with network interactions
• de Sitter-invariant special relativity and the dark energy problem
• False Vacuum in the Supersymmetric Mass Varying Neutrinos Model
• Dynamics of Multi-Component, Multi-Field Quintessence
• Lensing-induced Non-Gaussian Signatures in the Cosmic Microwave Background
• A WDM model for the evolution of galactic halos
• Constraints on the unified dark energy-dark matter model from latest observational data
• Baryonic and Leptonic GeV Dark Matter
• Thermodynamical study of FRW universe in Quasi-Topological Theory
• The torsion cosmology in Kaluza-Klein theory
• Gravitational lensing by a black hole with torsion
• The reheating constraints to natural inflation in Horndeski gravity
• Self-similar cosmologies in 5D: Our universe as a topological separation from an empty 5D Minkowski space
• Warm Dark Matter versus Bumpy Power Spectra
• Closed inflationary universe models in Braneworld Cosmology
• SuperBIT Superpressure Flight Instrument Overview and Performance: Near diffraction-limited Astronomical Imaging from the Stratosphere
• Interacting Induced Dark Energy Model
• How accurately can suborbital experiments measure the CMB?
• Gödel-type Solutions in Cubic Galileon Gravity
• Determining the Equation of State of the Expanding Universe Using a New Independent Variable
• 20+ years of Inflation
• Role of a periodic varying deceleration parameter in Particle creation with higher dimensional FLRW Universe
• Bulk scalar field in brane-worlds with induced gravity inspired by the $\mathcal{L}(R)$ term
• Inhomogenous Primordial Baryon Distributions on Sub-Galactic Scales: High-z Galaxy Formation with WDM
• Kinetic inductance detectors for millimeter and submillimeter astronomy / Détecteurs à inductance cinétique pour l'astronomie millimétrique et sub-millimétrique
• Probing Composite Gravity in Colliders
• Degree of randomness: numerical experiments for astrophysical signals
• A Newtonian Model for the Quantum Gravitational Back-Reaction on Inflation
• The power spectrum of the cosmic microwave background Kolmogorov maps: possible clue to correlation of voids
• Peculiarities of anisotropy and polarization as an indicator of noises in the CMB maps
• Phase structure of the $O(2)$ ghost model with higher-order gradient term
• Arrows of Time and Chaotic Properties of the Cosmic Background Radiation
• Phantom Mimicry on the Normal Branch of a DGP-inspired Braneworld Scenario with Curvature Effect
• Unification of Gravitation, Gauge Field and Dark Energy
• Classification of multifluid CP world models
• The establishment of the Standard Cosmological Model through observations
• Anisotropic background for two fluids: matter and holographic dark energy
• Gauss-Bonnet Braneworld Cosmology with Modified Induced Gravity on the Brane
• Accelerated closed universes in scalar-tensor theories
• Cosmological Fluctuations on the Light Cone
• Electron-photon interaction in de Sitter ambient space formalism
• Primordial Gaussian Fluctuations from Cosmic Defects
• Vacuum Decay Constraints on a Cosmological Scalar Field
• Study of thermal stability for different dark energy models
• Cosmic Equation of State and Advanced LIGO Type Gravity Wave Experiments
• Hybrid Inflation, Dark Energy And Dark Matter
• Entropy in locally-de Sitter spacetimes
• Exact solution to perturbative conformal cosmology from recombination until the current era
• CMB and LSS constraints on a single-field model of inflation
• Distance measurements as a probe of cosmic acceleration
• A Study of Universal Thermodynamics in Massive Gravity: Modified Entropy on the Horizons
• Overconstrained dynamics in galaxy redshift surveys
• Cosmological constraints from galaxy clustering
• Classical and quantum quintessence cosmology
• Likelihood distribution for models with cosmological constant from COBE data
• In Support of Inflation
• Inflation via logarithmic entropy-corrected holographic dark energy model
• Scattering of scalar perturbations with cosmological constant in low-energy and high-energy regimes
• The Fourth Gravity Test and Quintessence Matter Field
• FLRW Cosmology of Induced Dark Energy Model and Open Universe
• Gravitational lenses in the dark Universe
• An Improved Framework for Quantum Gravity
• Constraining decaying dark energy density models with the CMB temperature-redshift relation
• Is non-particle dark matter equation of state parameter evolving with time?
• Polarization tensor in de Sitter gauge gravity
• Observational constraints in late time for an axially symmetric transitioning model with bulk viscous fluid
• Application of Physics-Informed Neural Networks in Removing Telescope Beam Effects
• f(R) in Holographic and Agegraphic Dark Energy Models and the Generalized Uncertainty Principle
• Self-similar cosmologies in 5D: spatially flat anisotropic models
• Cosmic Strings and Quintessence
• The effect of signal digitisation in CMB experiments
• Periodic distribution of galaxies in generalized scalar tensor theory
• Acoustic Neutrino Detection In a Adriatic Multidisciplinary Observatory (ANDIAMO)
• Multi-component power spectra estimation method for multi-detector observations of the Cosmic Microwave Background
• Can MONDian vector theories explain the cosmic speed up ?
• Phantom scalar emission in the Kerr black hole spacetime
• Inhomogeneous structure formation may alleviate need for accelerating universe
• An overview of the current status of CMB observations
• The Dynamics of Brane-World Cosmological Models
• The ${\Omega }_{DE}-{\Omega }_M$ Plane in Dark Energy Cosmology
• The Higgs field and the resolution of the Cosmological Constant Paradox in the Weyl geometrical Universe
• Evolution of spherical overdensities in new agegraphic dark energy model
• Cosmic Initial Conditions for a Habitable Universe
• The Cosmic Microwave Background anisotropies: open problems
• Variation of the Fine-Structure Constant from the de Sitter Invariant Special Relativity
• Statistical evaluation of the observational information on ${\Omega }_m$ and ${\Omega }_{\Lambda }$
• A theoretically-explained new-variant of Modified-Newtonian-Dynamics (MOND)
• Interacting dark fluid in the universe bounded by event horizon : A non-equilibrium prescription
• Equilibrium configurations in the dynamics of irrotational dust matter
• The effect of the cosmological constant on gravitational wave quadrupole signal
• Searching for a solution to the cosmological constant problem - a toy model
• Cosmological constant and the fate of the DDM theory
• Assisted inflation in Bianchi VI0 cosmologies
• Matching the observed cosmological constant with vacuum energy density in AdS
• Homology reveals significant anisotropy in the cosmic microwave background
• Gravastar-like black hole solutions in $q$-theory
• Vacuum Energy Density and Cosmological Constant in dS Brane World
• Imprint of galactic rotation curves and metric fluctuations on the recombination era anisotropy
• Constraining Lambda using cluster quadrupoles
• Goodness--of--fit Statistics and CMB Data Sets
• On the contribution of density perturbations and gravitational waves to the lower order multipoles of the Cosmic Microwave Background Radiation
• Shedding Light on Dark Sectors with Gravitational Waves
• Do data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• A Modified chi^2-Test for CMB Analyses
• Paths of Friedmann-Robertson-Walker brane models
• Dynamical Shortcomings in the Generalized SU(2) Proca Theory: Challenges for Cosmic Acceleration
• Excessive shift of the CMB acoustic peaks of the Cold Spot area
• Stability of HDE model with sign-changeable interaction in Brans-Dicke theory
• Reply to "On scaling solutions with a dissipative fluid"
• Dark Energy Density in Brane World
• Primordial Nucleosynthesis, Cosmic Microwave Background and Neutrinos
• Supergravity models of Quintessence and Supersymmetry breaking
• Incompatibility of a comoving Ly-alpha forest with supernova-Ia luminosity distances
• On Local Approximations to the Nonlinear Evolution of Large-Scale Structure
• Stellar structure of quark stars in a modified Starobinsky gravity
• On the Casimir energy for a massive quantum scalar field and the Cosmological constant
• Testing CMB polarization data using position angles
• On the Cross-Correlation between Dark Matter Distribution and Secondary CMB Anisotropies by Ionized Intergalactic Medium
• Interacting Dark Energy and Its Implications for Unified Dark Sector
• Physics of Cosmic Microwave Background anisotropies and primordial fluctuations
• Cosmic Microwave Background anisotropies: the power spectrum and beyond
• (P)reheating Effects of the Kähler Moduli Inflation I Model
• Revisiting Barrow's Graduated Inflationary Universe: A Warm perspective
• A Null Test of the Metric Nature of the Cosmic Acceleration
• Determination of cosmology and evolution from K-band magnitude-redshift and number count observations
• Space-time singularities and the theory of retracts
• Particle mixing as possible explanation of the dark energy conundrum
• Cosmological Constraints on the Undulant Universe
• Tachyonic Universes in Patch Cosmologies with $\Omega >1$
• On the width of the last scattering surface
• De Sitter scalar-spinor interaction in Minkowski limit
• Quintessence and the first Doppler peak
• Fluids in cosmology
• Forecasting isocurvature models with CMB lensing information: axion and curvaton scenarios
• Magnetic Branes in Brans-Dicke-Maxwell Theory
• Post-Newtonian Gravitational Waves with cosmological constant $\Lambda$ from the Einstein-Hilbert theory
• Photon decaying in de Sitter universe
• Revisiting Agegraphic Dark Energy in Brans-Dicke Cosmology
• CMB with Quintessence: Analytic Approach and CMBFAST
• Can hyperbolic phase of Brans-Dicke field account for Dark Matter?
• Cosmological model with Born-Infeld type scalar field
• An accelerated closed universe
• The Effect of Interstellar Absorption on Measurements of the Baryon Acoustic Peak in the Lyman-α Forest
• How much will we learn from the CMB ?
• The Cosmic Background Radiation circa nu2K
• Extended black hole cosmologies in de Sitter space
• Density pertubation of unparticle dark matter in the flat Universe
• Can accelerated expansion of the universe be due to spacetime vorticity?
• Cosmological consequences of an inhomogeneous space-time
• Cosmological predictions from the Misner brane
• Matter loops corrected modified gravity in Palatini formulation
• A new topological perspective of expanding space-times with applications to cosmology
• Quantum Fluctuations of the Gravitational Field and Propagation of Light: a Heuristic Approach
• A Study on Ricci Dark Energy in Bulk-Brane Interaction
• A causal model for a closed universe
• Is the $\Lambda$CDM Model in Crisis?
• Cosmological implications from the observed properties of CMB
• The Lambert $W$ equation of state in light of DESI BAO
• Maps of the Cosmos: The Cosmic Microwave Background
• Unifying the Dark Sector with the New Generalized Chaplygin Gas: Observational Constraints
• Viaggiu holographic dark energy in light of DESI DR2
• Seeable universe and its accelerated expansion: an observational test
• Scale Dependence of Dark Energy Antigravity
• Verifying the use of supernovae as probes of the cosmic expansion
• Observers in an accelerated universe
• Cosmological models with the spinor and non-minimally interacting scalar field
• Late time cosmological solutions in $f(R,T)$ gravity in a viscous Universe
• $G_3$ -- interacting scalar tensor dark energy
• Recent Advances in Large-Scale Structure and Galaxy Formation Studies
• Holographic dark energy models with Interactions and entropy corrections for different cutoffs in the Brans-Dicke cosmology
• On the accelerated expansion of the cosmos
• Energy conditions and entropy density of the universe
• Quintessence reconstruction of interacting HDE in a non-flat universe
• The Cosmic Microwave Background
• Quasinormal Modes of Black holes in the generalized Schwarzschild-de Sitter solution of $f(R)$ gravity
• Lepton asymmetries from neutrino oscillations
• The spatial clustering of radio sources in NVSS and FIRST; implications for galaxy clustering evolution
• Evolution of entropic dark energy and its phantom nature
• Probing the Neutrino Seesaw Scale with Gravitational Waves