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