Cosmological parameters from SDSS and WMAP

Abstract

We measure cosmological parameters using the three-dimensional power spectrum P(k) from over 200,000 galaxies in the Sloan Digital Sky Survey (SDSS) in combination with WMAP and other data. Our results are consistent with a ``vanilla'' flat adiabatic Lambda-CDM model without tilt (n=1), running tilt, tensor modes or massive neutrinos. Adding SDSS information more than halves the WMAP-only error bars on some parameters, tightening 1 sigma constraints on the Hubble parameter from h~0.74+0.18-0.07 to h~0.70+0.04-0.03, on the matter density from Omega_m~0.25+/-0.10 to Omega_m~0.30+/-0.04 (1 sigma) and on neutrino masses from <11 eV to <0.6 eV (95%). SDSS helps even more when dropping prior assumptions about curvature, neutrinos, tensor modes and the equation of state. Our results are in substantial agreement with the joint analysis of WMAP and the 2dF Galaxy Redshift Survey, which is an impressive consistency check with independent redshift survey data and analysis techniques. In this paper, we place particular emphasis on clarifying the physical origin of the constraints, i.e., what we do and do not know when using different data sets and prior assumptions. For instance, dropping the assumption that space is perfectly flat, the WMAP-only constraint on the measured age of the Universe tightens from t0~16.3+2.3-1.8 Gyr to t0~14.1+1.0-0.9 Gyr by adding SDSS and SN Ia data. Including tensors, running tilt, neutrino mass and equation of state in the list of free parameters, many constraints are still quite weak, but future cosmological measurements from SDSS and other sources should allow these to be substantially tightened.

Minor revisions to match accepted PRD version. SDSS data and ppt figures available at http://www.hep.upenn.edu/~max/sdsspars.html

References in corpus (95)

• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Cosmological parameters from CMB and other data: a Monte-Carlo approach
• Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
• The 2dF Galaxy Redshift Survey: Spectra and redshifts
• Phantom Energy and Cosmic Doomsday
• Stable clustering, the halo model and nonlinear cosmological power spectra
• Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
• The 3D power spectrum of galaxies from the SDSS
• Cosmological Results from High-z Supernovae
• The u'g'r'i'z' Standard Star Network
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation
• The Mass Function of an X-Ray Flux-Limited Sample of Galaxy Clusters
• Spectroscopic Target Selection for the Sloan Digital Sky Survey: The Luminous Red Galaxy Sample
• The First Data Release of the Sloan Digital Sky Survey
• Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization
• Astrometric Calibration of the Sloan Digital Sky Survey
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum
• The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe
• DASI First Results: A Measurement of the Cosmic Microwave Background Angular Power Spectrum
• A photometricity and extinction monitor at the Apache Point Observatory
• The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe
• Galaxy Clustering in Early SDSS Redshift Data
• The significance of the largest scale CMB fluctuations in WMAP
• How long before the end of inflation were observable perturbations produced?
• An Efficient Algorithm for Positioning Tiles in the Sloan Digital Sky Survey
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Parameter Estimation Methodology
• The State of the Dark Energy Equation of State
• A High Spatial Resolution Analysis of the MAXIMA-1 Cosmic Microwave Background Anisotropy Data
• Cosmological bounds on neutrino degeneracy improved by flavor oscillations
• High Resolution Observations of the CMB Power Spectrum with ACBAR
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks
• Measuring ${\Omega }_m$ with the ROSAT Deep Cluster Survey
• Primordial Nucleosynthesis in Light of WMAP
• Reconstructing the primordial power spectrum
• Large Scale Cosmic Microwave Background Anisotropies and Dark Energy
• The White Dwarf Cooling Sequence of the Globular Cluster Messier 4
• Detection of the ISW and SZ effects from the CMB-Galaxy correlation
• Precision Cosmology? Not Just Yet
• Determining Neutrino Mass from the CMB Alone
• The 2dF Galaxy Redshift Survey: The amplitudes of fluctuations in the 2dFGRS and the CMB, and implications for galaxy biasing
• Cosmological Parameters from Cosmic Background Imager Observations and Comparisons with BOOMERANG, DASI, and MAXIMA
• Analytical treatment of neutrino asymmetry equilibration from flavour oscillations in the early universe
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• Neutrino masses and the number of neutrino species from WMAP and 2dFGRS
• Weak Lensing Results from the 75 Square Degree CTIO Survey
• Constraints on Omega_m and sigma_8 from weak lensing in RCS fields
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• The REFLEX Galaxy Cluster Survey VII: Omega_m and sigma_8 from cluster abundance and large-scale clustering
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• Efficient Cosmological Parameter Estimation from Microwave Background Anisotropies
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• Normal Parameters for an Analytic Description of the CMB Cosmological Parameter Likelihood
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• Nucleosynthesis, Reionization, and the Mass Function of the First Stars
• Phantom Cosmologies
• Attractor Solutions in f(T) Cosmology
• Markov Chain Monte Carlo Exploration of Minimal Supergravity with Implications for Dark Matter
• LXCDM: a cosmon model solution to the cosmological coincidence problem?
• Neutrinoless Double Beta Decay
• Two-Field Quintom Models in the w-w' Plane
• Density perturbations in general modified gravitational theories
• Gauged Supergravities
• Exclusion Limits on the WIMP-Nucleon Cross-Section from the First Run of the Cryogenic Dark Matter Search in the Soudan Underground Lab
• Cosmology with a Variable Chaplygin Gas
• Density perturbations in f(R) gravity theories in metric and Palatini formalisms
• Density perturbations in generalized Einstein scenarios and constraints on nonminimal couplings from the Cosmic Microwave Background
• Cosmological Constraints on $f(G)$ Dark Energy Models
• Instrument, Method, Brightness and Polarization Maps from the 2003 flight of BOOMERanG
• Observational $H(z)$ Data and Cosmological Models
• The Cosmological Dynamics of Interacting Holographic Dark Energy Model
• Clustering Fossils from the Early Universe
• Some Aspects of Thermal Leptogenesis
• Quintom model with O($N$) symmetry
• Clustering of quasars in SDSS-IV eBOSS : study of potential systematics and bias determination
• Cosmic Calibration: Constraints from the Matter Power Spectrum and the Cosmic Microwave Background
• Dark Energy Constraints from the CTIO Lensing Survey
• Compressed supersymmetry and natural neutralino dark matter from top squark-mediated annihilation to top quarks
• Dark Matter, Light Stops and Electroweak Baryogenesis
• The Transit Light Curve Project. III. Tres Transits of TrES-1
• CMB multipole measurements in the presence of foregrounds
• Agegraphic dark energy as a quintessence
• The Topology of the Cosmic Web in Terms of Persistent Betti Numbers
• Constraints on dark matter scenarios from measurements of the galaxy luminosity function at high redshifts
• Probing neutrino masses with future galaxy redshift surveys
• Inflation in Realistic D-Brane Models
• Stability of the Einstein static Universe in $f(R,T)$ gravity
• The History of Cosmological Star Formation: Three Independent Approaches and a Critical Test Using the Extragalactic Background Light
• The Transit Light Curve Project. XIII. Sixteen Transits of the Super-Earth GJ 1214b
• Integrated Sachs-Wolfe effect in Cross-Correlation: The Observer's Manual
• Holographic tachyon model
• Uses of zeta regularization in QFT with boundary conditions: a cosmo-topological Casimir effect
• Cosmo-dynamics and dark energy with non-linear equation of state: a quadratic model
• Primordial non-Gaussianities in general modified gravitational models of inflation
• On the Inference of Thermal Inversions in Hot Jupiter Atmospheres
• Quantitative Spectroscopy of Blue Supergiant Stars in the Disk of M81: Metallicity, Metallicity Gradient and Distance
• The Cluster Mass Function from Weak Gravitational Lensing
• Current cosmological bounds on neutrino masses and relativistic relics
• The Transit Light Curve Project. VII. The Not-So-Bloated Exoplanet HAT-P-1b
• New constraints on MOND from galaxy clusters
• Noether Symmetry Approach in f(R) Tachyon Model
• Interacting agegraphic dark energy models in non-flat universe
• A Note on Tsallis Holographic Dark Energy
• Dark energy models with variable equation of state parameter
• Can superhorizon cosmological perturbations explain the acceleration of the universe?
• Probing for dynamics of dark energy and curvature of universe with latest cosmological observations
• The influence of non-uniform reionization on the CMB
• $f(T)$ cosmology via Noether symmetry
• Observing Dark Energy Dynamics with Supernova, Microwave Background and Galaxy Clustering
• Keck Laser Guide Star Adaptive Optics Monitoring of 2MASS J1534-2952AB: First Dynamical Mass Determination of a Binary T Dwarf
• Age Problem in the Holographic Dark Energy Model
• Mismatch between X-ray and emission-weighted temperatures in galaxy clusters: cosmological implications
• Holographic modified gravity
• Gravitational Leptogenesis and Its Signatures in CMB
• Friedmann cosmology with decaying vacuum density
• Quintessence reconstruction of the new agegraphic dark energy model
• Inhomogenized sudden future singularities
• DBI-essence
• Transiting exoplanets from the CoRoT space mission. XV. CoRoT-15b: a brown dwarf transiting companion
• Models of inflation liberated by the curvaton hypothesis
• Observational constraints on holographic dark energy with varying gravitational constant
• Constraining Neutrino Masses by CMB Experiments Alone
• Information content of the non-linear matter power spectrum
• Some Issues Concerning Holographic Dark Energy
• Quintessential Inflation on the Brane and the Relic Gravity Wave Background
• Cosmology with High-redshift Galaxy Survey: Neutrino Mass and Inflation
• Cosmological parameters from strong gravitational lensing and stellar dynamics in elliptical galaxies
• Reheating via a generalized non-minimal coupling of curvature to matter
• An analytic model for interacting dark energy and its observational constraints
• Curvature vs Distances: testing the FLRW cosmology
• SDSS Galaxy Clustering: Luminosity & Colour Dependence and Stochasticity
• Detection Rate Estimates of Gravity-waves Emitted During Parabolic Encounters of Stellar Black Holes in Globular Clusters
• Breaking the Degeneracies Between Cosmology and Galaxy Bias
• Statefinders, higher-order energy conditions and sudden future singularities
• Local Voids as the Origin of Large-angle Cosmic Microwave Background Anomalies: The Effect of a Cosmological Constant
• A new interacting two fluid model and its consequences
• Constraints on the Sound Speed of Dynamical Dark Energy
• Are peculiar velocity surveys competitive as a cosmological probe?
• Confronting Braneworld Cosmology with Supernova data and Baryon Oscillations
• The Supersymmetric Origin of Matter
• Dynamics of an Interacting Barrow Holographic Dark Energy Model and its Thermodynamic Implications
• Viscous dark fluid universe
• Anisotropic cosmological models in $f(R,T)$ gravity with variable deceleration parameter
• Bayesian evidence as a tool for comparing datasets
• Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter
• Highly Accreting Quasars: Sample Definition and Possible Cosmological Implications
• Physical Characteristics and Maximum Allowable Mass of Hybrid Star in the Context of $f(Q)$ Gravity
• Features of holographic dark energy under the combined cosmological constraints
• Holographic dark energy in Brans-Dicke cosmology with chameleon scalar field
• Cosmology and the Halo Occupation Distribution from Small-Scale Galaxy Clustering in the Sloan Digital Sky Survey
• The Rotation Velocity Attributable to Dark Matter at Intermediate Radii in Disk Galaxies
• The Hubble Constant
• The supernova Hubble diagram for off-center observers in a spherically symmetric inhomogeneous universe
• Primordial Neutrinos
• Exorcising w < -1
• Instability of QCD ghost dark energy model
• Self-gravitating system made of axions
• On holographic dark-energy models
• The WiggleZ Dark Energy Survey: the selection function and z=0.6 galaxy power spectrum
• Can a matter-dominated model with constant bulk viscosity drive the accelerated expansion of the universe?
• A New Limit on the Neutrinoless DBD of 130Te
• Tracing the Reionization-Epoch Intergalactic Medium with Metal Absorption Lines
• Model independent analysis of dark energy I: Supernova fitting result
• The GALEX Arecibo SDSS survey: III. Evidence for the Inside-Out Formation of Galactic Disks
• Assessment of the Information Content of the Power Spectrum and Bispectrum
• Holographic dark energy in a cyclic universe
• The Beginning and Evolution of the Universe
• Thermodynamical Interpretation of the Interacting Holographic Dark Energy Model in a non-flat Universe
• Tension and Systematics in the Gold06 SnIa Dataset
• A transit timing analysis of nine RISE light curves of the exoplanet system TrES-3
• WIMP Dark Matter and the QCD Equation of State
• Dynamics of Interacting Quintessence Models: Observational Constraints
• Departures from the FLRW Cosmological Model in an Inhomogeneous Universe: A Numerical Examination
• Some remarks on the dynamical systems approach to fourth order gravity
• Exploring a matter-dominated model with bulk viscosity to drive the accelerated expansion of the Universe
• Measuring the cosmic evolution of dark energy with baryonic oscillations in the galaxy power spectrum
• Constraining f(T) teleparallel gravity by Big Bang Nucleosynthesis
• Second Order General Slow-Roll Power Spectrum
• Constraints on the sound speed of dark energy
• Noether symmetry in $f(R)$ cosmology
• Phantom damping of matter perturbations
• Modified Chaplygin Gas Cosmology
• Phantom Friedmann Cosmologies and Higher-Order Characteristics of Expansion
• Evolution of a Schwarzschild Black Hole in Phantom-like Chaplygin gas Cosmologies
• Statistical Analysis of Galaxy Surveys-II. The 3-point galaxy correlation function measured from the 2dFGRS
• Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints
• Stability of a non-minimally conformally coupled scalar field in F(T) cosmology
• The origin of polar ring galaxies: evidence for galaxy formation by cold accretion
• The Nuclear Cluster of the Milky Way: Total Mass and Luminosity (long version)
• Accretion, feedback and galaxy bimodality: a comparison of the GalICS semi-analytic model and cosmological SPH simulations
• Two-Fluid Scenario for Dark Energy Models in an FRW Universe-Revisited
• Evolving Newton's Constant, Extended Gravity Theories and SnIa Data Analysis
• Observational bounds on the cosmic radiation density
• Cosmokinetics: A joint analysis of Standard Candles, Rulers and Cosmic Clocks
• Future singularities and Teleparallelism in Loop Quantum Cosmology
• Cosmological parameter estimation using Very Small Array data out to l=1500
• Noether symmetry of F(T) cosmology with quintessence and phantom scalar fields
• Direct Detection of Dark Matter Rates for Various Wimps
• Examining the cosmic acceleration with the latest Union2 supernova data
• Measuring neutrino masses and dark energy with weak lensing tomography
• Reconstructing the primordial power spectrum - a new algorithm
• Cosmic Calibration
• New holographic scalar field models of dark energy in non-flat universe
• Interacting Ghost Dark Energy in Non-Flat Universe
• Escaping the Big Rip?
• Wide Angle Redshift Distortions Revisited
• General analytic formulae for attractor solutions of scalar-field dark energy models and their multi-field generalizations
• Photon-axion conversion as a mechanism for supernova dimming: Limits from CMB spectral distortion
• Cosmological consequences of an adiabatic matter creation process
• Non-linear Structure Formation in Cosmologies with Early Dark Energy
• Interesting radiative patterns of neutrino mass in an SU(3)_C X SU(3)_L X U(1)_X model with right-handed neutrinos
• Cosmic history of viable exponential gravity: Equation of state oscillations and growth index from inflation to dark energy era
• Dynamical dark energy or variable cosmological parameters?
• Current Observational Constraints to Holographic Dark Energy Model with New Infrared cut-off via Markov Chain Monte Carlo Method
• The Transit Light Curve (TLC) Project. II. Two Transits of the Exoplanet OGLE-TR-111b
• Cosmological Constraints on the Sign-Changeable Interactions
• Cosmological dynamics of tachyonic teleparallel dark energy
• Spin-Orbit Alignment for the Eccentric Exoplanet HD 147506b
• On the co-existence of matter dominated and accelerating solutions in f(G)-gravity
• Lightest Neutralino in Extensions of the MSSM
• Strange stars in Krori-Barua space-time under f(R; T) gravity
• Transition from quintessence to phantom phase in quintom model
• A Third Hot White Dwarf Companion Detected by Kepler
• Improved Measurements of the CMB Power Spectrum with ACBAR
• The Transit Ingress and the Tilted Orbit of the Extraordinarily Eccentric Exoplanet HD 80606b
• Cosmological Applications of Pade Approximant
• Cosmological Parameters from the Comparison of the 2MASS Gravity Field with Peculiar Velocity Surveys
• If Gauss-Bonnet interaction plays the role of dark energy
• Internal space structure generalization of the quintom cosmological scenario
• Bianchi Type-I Anisotropic Dark Energy Models with Constant Deceleration Parameter
• Redshift-Space Distortions with the Halo Occupation Distribution I: Numerical Simulations
• The stability of the Einstein static state in $f(T)$ gravity
• Neutrino masses and CDM in a non-supersymmetric model
• Correlated Primordial Perturbations in Light of CMB and LSS Data
• Non-minimally Coupled Quintom Model Inspired by String Theory
• VLT transit and occultation photometry for the bloated planet CoRoT-1b
• Discovery of a Third Transiting Planet in the Kepler-47 Circumbinary System
• New Neutrino Mass Bounds from Sloan Digital Sky Survey III Data Release 8 Photometric Luminous Galaxies
• Cosmological Inflation in f(Q, T) Gravity
• Effective $F(T)$ gravity from the higher-dimensional Kaluza-Klein and Randall-Sundrum theories
• CosmoHammer: Cosmological parameter estimation with the MCMC Hammer
• General Non-minimal Kinetic coupling to gravity
• SOPHIE velocimetry of Kepler transit candidates XII. KOI-1257 b: a highly eccentric three-month period transiting exoplanet
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: weighing the neutrino mass using the galaxy power spectrum of the CMASS sample
• Leptogenesis beyond the limit of hierarchical heavy neutrino masses
• Comparison of Approaches to Quantum Correction of Black Hole Thermodynamics
• Gravity on codimension 2 brane worlds
• A Note on Crossing the Phantom Divide in Hybrid Dark Energy Model
• Dynamics of Particles Around a Schwarzschild-like Black Hole in the Presence of Quintessence and Magnetic Field
• Reconstruction of Deceleration Parameters from Recent Cosmic Observations
• Indirect signals from light neutralinos in supersymmetric models without gaugino mass unification
• Weighing Neutrinos with Galaxy Cluster Surveys
• Cosmological Implications of the Uncertainty in H- Destruction Rate Coefficients
• New agegraphic dark energy in Horava-Lifshitz cosmology
• Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to Constrain Dark Energy
• Comparing approximate methods for mock catalogues and covariance matrices II: Power spectrum multipoles
• The Weak Lensing Signal and the Clustering of BOSS Galaxies I: Measurements
• Constraints on the identity of the dark matter from strong gravitational lenses
• Thermodynamics second law and $\omega =-1$ crossing(s) in interacting holographic dark energy model
• Supernovae constraints on models of dark energy revisited
• Substructure and galaxy formation in the Copernicus Complexio warm dark matter simulations
• Unraveling the effective fluid approach for $f(R)$ models in the subhorizon approximation
• Dynamical behavior of generic quintessence potentials: constraints on key dark energy observables
• Testing the dark energy with gravitational lensing statistics
• Neutrino Mixing Predictions of a Minimal SO(10) Model with Suppressed Proton Decay
• Supermassive black holes from primordial black hole seeds
• Three-generation flavor transitions and decays of supernova relic neutrinos
• Reconstruction of Hessence Dark Energy and the Latest Type Ia Supernovae Gold Dataset
• K-Chameleon and the Coincidence Problem
• Dark energy transition between quintessence and phantom regimes - an equation of state analysis
• Cosmological electromagnetic fields and dark energy
• Wide Angle Effects in Future Galaxy Surveys
• A model with interaction of dark components and recent observational data
• Ground-based detection of thermal emission from the exoplanet WASP-19b
• Reconstruction of general scalar-field dark energy models
• A clear and measurable signature of modified gravity in the galaxy velocity field
• Dynamics of f(R)-cosmologies containing Einstein static models
• Cross-correlation of CMB with large-scale structure: weak gravitational lensing
• A Modified Holographic Dark Energy Model with Infrared Infinite Extra Dimension(s)
• Constraints on Distance Duality Relation from Sunyaev Zel'dovich Effect and Chandra X-ray measurements
• Primordial helium recombination I: feedback, line transfer, and continuum opacity
• Another Look at Minimal Lepton Flavour Violation, l_i -> l_j gamma, Leptogenesis, and the Ratio M_nu/ Lambda_LFV
• Noether Symmetry Approach in $f(\mathcal{G},T)$ Gravity
• Interacting model of new agegraphic dark energy: Cosmological evolution and statefinder diagnostic
• Indication for Primordial Anisotropies in the Neutrino Background from WMAP and SDSS
• Testing Bekenstein's Relativistic MOND gravity with Lensing Data
• Cosmological Lepton Asymmetry, Primordial Nucleosynthesis, and Sterile Neutrinos
• Deflection of light by black holes and massless wormholes in massive gravity
• Two photon annihilation of Kaluza-Klein dark matter
• Top transport in electroweak baryogenesis
• A Possible Spin-Orbit Misalignment in the Transiting Eccentric Planet HD 17156b
• $H_0$ tension as a hint for a transition in gravitational theory
• Higher order corrections of the extended Chaplygin gas cosmology with varying $G$ and $\Lambda$
• Baryon Dynamics, Dark Matter Substructure, and Galaxies
• Realistic cosmological scenario with non-minimal kinetic coupling
• X-ray Preionisation Powered by Accretion on the First Black Holes. II: Cosmological Simulations and Observational Signatures
• On the generalised Chaplygin gas: worse than a big rip or quieter than a sudden singularity?
• Direct reconstruction of the quintessence potential
• Covariance of cross-correlations: towards efficient measures for large-scale structure
• Constraints on the coupled quintessence from cosmic microwave background anisotropy and matter power spectrum
• Information content of the non-linear power spectrum: the effect of beat-coupling to large scales
• Gravitational Leptogenesis and Neutrino Mass Limit
• Sterile Neutrinos in Light of Recent Cosmological and Oscillation Data: a Multi-Flavor Scheme Approach
• An Independent Analysis of Kepler-4b through Kepler-8b
• Keck Laser Guide Star Adaptive Optics Monitoring of the M8+L7 Binary LHS 2397aAB: First Dynamical Mass Benchmark at the L/T Transition
• Cosmological Models and Gamma-Ray Bursts Calibrated by Using Pade Method
• Relativistic Stars in dRGT Massive Gravity
• Dark energy model with higher derivative of Hubble parameter
• Testing homogeneity on large scales in the Sloan Digital Sky Survey Data Release One
• Neutrino Masses from Cosmological Probes
• Time Lumps in Nonlocal Stringy Models and Cosmological Applications
• Kination Dominated Reheating and Cold Dark Matter Abundance
• Can Gamma-Ray Bursts Be Used to Measure Cosmology? A Further Analysis
• Bianchi Type I Cosmology in Generalized Saez-Ballester Theory via Noether Gauge Symmetry
• Imprints of Dark Energy on Cosmic Structure Formation I) Realistic Quintessence Models and the Non-Linear Matter Power Spectrum
• Quintessential Kination and Cold Dark Matter Abundance
• First underground results with NEWAGE-0.3a direction-sensitive dark matter detector
• Discovery of Two Gravitationally Lensed Quasars with Image Separations of 3 Arcseconds from the Sloan Digital Sky Survey
• Empirical Constraints on Trojan Companions and Orbital Eccentricities in 25 Transiting Exoplanetary Systems
• A parametrization of the growth index of matter perturbations in various Dark Energy models and observational prospects using a Euclid-like survey
• Some Exact Solutions in $f(\mathcal{G},T)$ Gravity via Noether Symmetries
• Tachyon warm inflationary universe models
• Theoretical Limits on the Equation-of-State Parameter of Phantom Cosmology
• Comparison of dark energy models after Planck 2015
• Cosmological dynamics with non-linear interactions
• Updated constraints on $f(\mathcal{R})$ gravity from cosmography
• CAIRNS: The Cluster And Infall Region Nearby Survey II. Environmental Dependence of Infrared Mass-to-Light Ratios
• Direction Dependence of the Deceleration Parameter
• Observational constraints on patch inflation in noncommutative spacetime
• LensExtractor: A Convolutional Neural Network in Search of Strong Gravitational Lenses
• The past and future dynamics of quintom dark energy models
• A new framework for studying spherically symmetric static solutions in f(R) gravity
• Diffuse inverse Compton and synchrotron emission from dark matter annihilations in galactic satellites
• The role of ionization electrons in direct dark matter detection
• The Clustering of MgII Absorption Systems at z=0.5 and Detection of Cold Gas in Massive Halos
• Updated parameters for the transiting exoplanet WASP-3b using RISE, a new fast camera for the Liverpool Telescope
• The State Equation of the Yang-Mills field Dark Energy Models
• Accretion and Evaporation of Modified Hayward Black Hole
• Beyond the perfect fluid hypothesis for dark energy equation of state
• Falsifying Paradigms for Cosmic Acceleration
• Non-local SFT Tachyon and Cosmology
• Measurement of Ω_m, Ω_Λ from a blind analysis of Type Ia supernovae with CMAGIC: Using color information to verify the acceleration of the Universe
• Baryon number asymmetry and dark matter in the neutrino mass model with an inert doublet
• Cosmological perturbations in warm inflationary models with viscous pressure
• Pilgrim Dark Energy
• Precise Radius Estimates for the Exoplanets WASP-1b and WASP-2b
• FRW Quantum Cosmology with a Generalized Chaplygin Gas
• On the Viability of Bianchi Type VIIh Models with Dark Energy
• Growth Index of DGP Model and Current Growth Rate Data
• Observing the clustering properties of galaxy clusters in dynamical dark-energy cosmologies
• Neutrino coupling to cosmological background: A review on gravitational Baryo/Leptogenesis
• Interacting dark matter and modified holographic Ricci dark energy plus a noninteracting cosmic component
• Theoretical uncertainty in baryon oscillations
• Morphologies and Color Gradients of Luminous Evolved Galaxies at z~1.5
• De Sitter Universe in Nonlocal Gravity
• Observational constraints on interacting Tsallis holographic dark energy models
• Holographic Dark Energy in Brans-Dicke Theory
• New agegraphic dark energy model with generalized uncertainty principle
• Analyze This! A Cosmological Constraint Package for CMBEASY
• Cosmological Evolution in f(R,T) theory with Collisional Matter
• Spherical collapse model with shear and angular momentum in dark energy cosmologies
• Impact of three years of data from the Wilkinson Microwave Anisotropy Probe on cosmological models with dynamical dark energy
• Enhanced polarization of CMB from thermal gravitational waves
• Aurora: A Generalised Retrieval Framework for Exoplanetary Transmission Spectra
• Towards a measurement of the spectral runnings
• Anatomy of F_D-Term Hybrid Inflation
• Relic Neutrino Absorption Spectroscopy
• Comparison of Standard Ruler and Standard Candle constraints on Dark Energy Models
• Dynamical Study of A1689 from Wide-Field VLT/VIMOS Spectroscopy: Mass Profile, Concentration Parameter, and Velocity Anisotropy
• Evolution and Dynamics of a Matter creation model
• Elastic Inflation
• Cosmological evolution in vector-tensor theories of gravity
• Ups and Downs in Dark Energy: phase transition in dark sector as a proposal to lessen cosmological tensions
• Axion constraints in non-standard thermal histories
• On Special Relativity with Cosmological Constant
• Revisit of the interacting holographic dark energy model after Planck 2015
• Rotational evolution of slow-rotators sequence stars
• Reionization, SLOAN, and WMAP: is the Picture Consistent?
• Determining the WIMP mass using direct detection experiments
• Constraining dark energy models using the lookback time to galaxy clusters and the age of the universe
• Constraining dark energy with Hubble parameter measurements: an analysis including future redshift-drift observations
• Probing the Epoch of Early Baryonic Infall Through 21cm Fluctuations
• Correlated isocurvature perturbations from mixed inflaton-curvaton decay
• Constraints on non-flat cosmologies with massive neutrinos after Planck 2015
• Atmospheric Retrieval of Exoplanets
• First season QUaD CMB temperature and polarization power spectra
• Genetic Algorithms and Supernovae Type Ia Analysis
• Two Upper Limits on the Rossiter-McLaughlin Effect, with Differing Implications: WASP-1 has a High Obliquity and WASP-2 is Indeterminate
• Constraints on reconstructed dark energy model from SN Ia and BAO/CMB observations
• Conserved Quantities in $f(R)$ Gravity via Noether Symmetry
• Running coupling: Does the coupling between dark energy and dark matter change sign during the cosmological evolution?
• Implications of a Stochastic Microscopic Finsler Cosmology
• Inflation by non-minimal coupling
• A 2% Distance to z = 0.35 by Reconstructing Baryon Acoustic Oscillations - III : Cosmological Measurements and Interpretation
• Limit on the Neutrino Mass from the WMAP Three Year Data
• Neutrino masses and cosmic radiation density: Combined analysis
• Galactic metric, dark radiation, dark pressure and gravitational lensing in brane world models
• Can dark energy be expressed as a power series of the Hubble parameter?
• An Independent Planet Search In The Kepler Dataset. II. An extremely low-density super-Earth mass planet around Kepler-87
• Test of the cosmic evolution using Gaussian processes
• NLTT 41135: a field M-dwarf + brown dwarf eclipsing binary in a triple system, discovered by the MEarth observatory
• Bulk viscous matter and recent acceleration of the Universe
• An Interacting Two-Fluid Scenario for Dark Energy in FRW Universe
• Observational constraints on braneworld inflation: the effect of a Gauss-Bonnet term
• Cosmological expansion and the uniqueness of gravitational action
• Inflationary cosmology in unimodular $F(T)$ gravity
• Dark Energy in Practice
• Distribution function approach to redshift space distortions. Part II: N-body simulations
• Pilgrim Dark Energy in $f(T,T_G)$ cosmology
• Dependence of the non-linear mass power spectrum on the equation of state of dark energy
• New constraints on SN Ia progenitor models
• Cosmic acceleration and crossing of w=-1 barrier in non-local Cubic Superstring Field Theory model
• Improved Limit on theta_{13} and Implications for Neutrino Masses in Neutrino-less Double Beta Decay and Cosmology
• Phased Breaking of mu-tau symmetry and Leptogenesis
• Interacting Ghost Dark Energy in Brans-Dicke Theory
• Imprint of the seesaw mechanism on feebly interacting dark matter and the baryon asymmetry
• Direct dark matter search by observing electrons produced in neutralino-nucleus collisions
• New Nuclear Physics for Big Bang Nucleosynthesis
• Age of High Redshift Objects - a Litmus Test for the Dark Energy Models
• Bayesian mass and age estimates for transiting exoplanet host stars
• Integration of inhomogeneous cosmological spacetimes in the BSSN formalism
• Correlation properties of the kinematic Sunyaev-Zel'dovich effect and implications for Dark Energy
• Observational signatures of anisotropic inflationary models
• Quintom dark energy models with nearly flat potentials
• Kinetic k-essence ghost dark energy model
• Analysis of Kepler's short-cadence photometry for TrES-2b
• Emergent Universe Scenario in the Einstein-Gauss-Bonnet Gravity with Dilaton
• Reconstruction of primordial density fields
• Did the Universe loiter at high redshifts ?
• Remarks on generalized Gauss-Bonnet dark energy
• WMAP constraints on inflationary models with global defects
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• Anisotropic dark energy model with a hybrid scale factor
• SOPHIE velocimetry of Kepler transit candidates. VIII. KOI-205 b: a brown-dwarf companion to a K-type dwarf
• A sub-horizon framework for probing the relationship between the cosmological matter distribution and metric perturbations
• A comparison of structure formation in minimally and non-minimally coupled quintessence models
• Is the Number of Giant Arcs in LCDM Consistent With Observations?
• A third alternative to explain recent observations: Future deceleration
• HI Signal from Reionization Epoch
• Bayesian analysis of Friedmannless cosmologies
• Large Scale Structure Constraints for a Class of f(R) Theories of Gravity
• Density Perturbations for Running Cosmological Constant
• The Nonlinear Cosmological Matter Power Spectrum with Massive Neutrinos I: The Halo Model
• Galaxy Size Problem at z=3: Simulated Galaxies Are Too Small
• The clustering of galaxies as a function of their photometrically-estimated atomic gas content
• The bouncing cosmology with $F(R)$ gravity and its reconstructing
• Testing for double inflation with WMAP
• The Clustering of Galaxies in the SDSS-III DR10 Baryon Oscillation Spectroscopic Survey: No Detectable Colour Dependence of Distance Scale or Growth Rate Measurements
• New observational constraints on $f(T)$ cosmology from radio quasars
• Cosmology with decaying tachyon matter
• Reconstruction of f(T) gravity from the Holographic dark energy
• Energy conditions in generalized teleparallel gravity models
• Leptogenesis and dark matter detection in a TeV scale neutrino mass model with inverted mass hierarchy
• Supernova constraints on decaying vacuum cosmology
• Features in Dark Energy Equation of State and Modulations in the Hubble Diagram
• A Running Spectral Index in Supersymmetric Dark-Matter Models with Quasi-Stable Charged Particles
• Shear and rotation in Chaplygin cosmology
• SN and BAO constraints on (new) polynomial dark energy parametrizations: current results and forecasts
• Extrasolar planet detection by binary stellar eclipse timing: evidence for a third body around CM Draconis
• Modified Gravity Explains Dark Matter?
• Thermal leptogenesis in a model with mass varying neutrinos
• Of pNGB QuiNtessence
• Overcoming the Circular Problem for γ-ray Bursts in Cosmological Global Fitting Analysis
• A New Equation of State for Dark Energy Model
• Interacting new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe
• Anomaly Induced Dark Matter Decay and PAMELA/ATIC Experiments
• Distribution function approach to redshift space distortions, Part III: halos and galaxies
• First Sources in Infrared Light: Stars, Supernovae and Miniquasars
• Measuring the Three-Dimensional Structure of Galaxy Clusters. II. Are clusters of galaxies oblate or prolate?
• Notes on dark energy interacting with dark matter and unparticle in loop quantum cosmology
• Non-parametric reconstruction of the primordial power spectrum at horizon scales from WMAP data
• Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters
• Accelerating dark energy models in bianchi Type-V space-time
• Efficient Cosmological Parameter Estimation with Hamiltonian Monte Carlo
• Cosmological Constraints on the Modified Entropic Force Model
• Toward a Universal Formulation of the Halo Mass Function
• Warm Inflation in $f(\mathcal{G})$ Theory of Gravity
• Constraints on a generalized deceleration parameter from cosmic chronometers
• Cosmo-dynamics and dark energy with a quadratic EoS: anisotropic models, large-scale perturbations and cosmological singularities
• Thermodynamic Behavior of particular $f(R,T)$ Gravity Models
• Early structure formation in quintessence models and its implications for cosmic reionisation from first stars
• How clustering dark energy affects matter perturbations
• Alleviation of Cosmic Age Problem In Interacting Dark Energy Model
• Limiting the dimming of distant type Ia supernovae
• Snyder's Model -- de Sitter Special Relativity Duality and de Sitter Gravity
• Accelerating universe from gravitational leakage into extra dimensions: confrontation with SNeIa
• On Precision Measurement of the Mean Curvature
• LCDM Model in f(T) Gravity: Reconstruction, Thermodynamics and Stability
• Cylindrical Solutions in Modified f(T) Gravity
• A Quintom scenario with mixed kinetic terms
• Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
• Galaxy redshift surveys selected by neutral hydrogen using FAST
• Extended quintessence with an exponential coupling
• Determining the WIMP mass from a single direct detection experiment, a more detailed study
• Warm inflation in the DGP brane-world model
• The SDSS Galaxy Angular Two-Point Correlation Function
• Star Models with Dark Energy
• Dynamical analysis and statefinder of Barrow holographic dark energy
• Models of Baryogenesis via Spontaneous Lorentz Violation
• Anisotropic perturbations due to dark energy
• Diphoton decays of stoponium at the Large Hadron Collider
• Stellar configurations in f(R) theories of gravity
• Modelling the rotational evolution of solar-like stars: the rotational coupling timescale
• A Bound Concerning Primordial Non-Gaussianity
• The generalized second law of gravitational thermodynamics on the apparent and event horizons in FRW cosmology
• The Chemical Properties of Milky Way and M31 Globular Clusters: II. Stellar Population Model Predictions
• A New Approach to Quintessence and a Solution of Multiple Attractors
• Phantom-like behaviour in dilatonic brane-world scenario with induced gravity
• Correspondence between entropy-corrected holographic and Gauss-Bonnet dark energy models
• Non-standard primordial fluctuations and nongaussianity in string inflation
• Cosmic tomographies: baryon acoustic oscillations and weak lensing
• Possible theoretical limits on holographic quintessence from weak gravity conjecture
• Stability analysis of the Tsallis holographic dark energy model
• Can a galaxy redshift survey measure dark energy clustering?
• The Monopole Moment of the Three-Point Correlation Function of the 2-degree Field Galaxy Redshift Survey
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• Interacting Entropy-Corrected Holographic Dark Energy and IR Cut-Off Length
• Holographic f(T)-gravity model with power-law entropy correction
• Observational constraints on Gauss-Bonnet cosmology
• Probing the curvature of the Universe from supernova measurement
• Inflation and dark energy arising from geometrical tachyons
• Holographic Dark Energy Model with Hubble Horizon as an IR Cut-off
• Reconstructing the Cosmic Expansion History up to Redshift z=6.29 with the Calibrated Gamma-Ray Bursts
• Learning from the Scatter in Type Ia Supernovae
• Black Hole Formation from Collapsing Dust Fluid in a Background of Dark Energy
• The electromagnetic dark sector
• Unveiling cosmography from the dark energy equation of state
• Dynamics of Quintom and Hessence Energies in Loop Quantum Cosmology
• Dark Energy Evolution and the Curvature of the Universe from Recent Observations
• Born in an Infinite Universe: a Cosmological Interpretation of Quantum Mechanics
• Generalized Holographic and Ricci Dark Energy Models
• Isotropy of the early universe from CMB anisotropies
• The XMM Cluster Survey: Forecasting cosmological and cluster scaling-relation parameter constraints
• Generalised DBI-Quintessence
• The Transit Light Curve Project. X. A Christmas Transit of HD 17156b
• Brane inflation in background supergravity
• LRS Bianchi type I universes exhibiting Noether symmetry in the scalar-tensor Brans-Dicke theory
• Lookback time bounds from energy conditions
• On the Past Asymptotic Dynamics of Non-minimally Coupled Dark Energy
• A transit timing analysis of seven RISE light curves of the exoplanet system HAT-P-3
• Gaussian processes reconstruction of dark energy from observational data
• Interacting Ricci Dark Energy with Logarithmic Correction
• Warm inflationary model in loop quantum cosmology
• APOSTLE Observations of GJ 1214b: System Parameters and Evidence for Stellar Activity
• Chaotic inflation in modified gravitational theories
• Current Observational Constraints on Cosmic Doomsday
• How to Distinguish Dark Energy and Modified Gravity?
• Neutrino masses, mixing and leptogenesis in TeV scale B-L extension of the standard model
• Enhancement of the annihilation of dark matter in a radiative seesaw model
• How far is it to a sudden future singularity of pressure?
• Effective gravitational coupling in modified teleparallel theories
• Dynamical system analysis for nonminimal torsion-matter coupled gravity
• Cheng-Weyl Vector Field and its Cosmological Application
• The Observed Growth of Massive Galaxy Clusters IV: Robust Constraints on Neutrino Properties
• Late universe dynamics with scale-independent linear couplings in the dark sector
• A Unified Approach to Variational Derivatives of Modified Gravitational Actions
• Constraints on cosmological models from lens redshift data
• The missing link: a nonlinear post-Friedmann framework for small and large scales
• Cosmographic parameters in model-independent approaches
• Tachyonic Teleparallel Dark Energy
• Analytic Methods for Cosmological Likelihoods
• Inflationary Potential Reconstruction for a WMAP Running Power Spectrum
• Direct versus indirect detection in mSUGRA with self-consistent halo models
• Transient cosmic acceleration from interacting fluids
• Constraints on Fundamental Cosmological Parameters with Upcoming Redshifted 21 cm Observations
• Constraints on f(R) theory and Galileons from the latest data of galaxy redshift surveys
• How close can an Inhomogeneous Universe mimic the Concordance Model?
• Cosmic evolution and thermal stability of Barrow holographic dark energy in nonflat Friedmann-Robertson-Walker Universe
• Cosmology with nonminimal kinetic coupling and a power-law potential
• Cosmological evolution and statefinder diagnostic for new holographic dark energy model in non flat universe
• Oscillations in the dark energy EoS: new MCMC lessons
• A Search for Dark Matter Annihilation with the Whipple 10m Telescope
• Dynamics of assisted quintessence
• 2HOT: An Improved Parallel Hashed Oct-Tree N-Body Algorithm for Cosmological Simulation
• Origin of holographic dark energy models
• Dark Matter in a Constrained NMSSM
• Bright optical dayside emission from extrasolar planet CoRoT-2b
• Structure of Dark Matter Halos in Warm Dark Matter models and in models with Long-Lived Charged Massive Particles
• Statefinder Analysis of f(T) Cosmology
• Cosmic vector for dark energy: constraints from SN, CMB and BAO
• The generalized second law in irreversible thermodynamics for the interacting dark energy in a non-flat FRW universe enclosed by the apparent horizon
• Interacting Energy Components and Observational $H(z)$ Data
• Generalized Chaplygin gas model, supernovae and cosmic topology
• Yang-Mills condensate dark energy coupled with matter and radiation
• On structure formation from a small-scales-interacting dark sector
• Holographic dark energy in Brans-Dicke theory with log correction
• Is cosmology compatible with sterile neutrinos?
• Tests of the CMB temperature-redshift relation, CMB spectral distortions and why adiabatic photon production is hard
• Cosmological perturbations in Palatini modified gravity
• Estimation of Cosmological Parameters from HI Observations of Post-reionization Epoch
• Correspondence between DBI-essence and Modified Chaplygin Gas and the Generalized Second Law of Thermodynamics
• Measuring our universe from galaxy redshift surveys
• Towards understanding the structure of voids in the cosmic web
• Non-universal gaugino masses, the supersymmetric little hierarchy problem, and dark matter
• Accelerating Universe in Hybrid and Logarithmic Teleparallel Gravity
• Reconstructing f(R) theory according to holographic dark energy
• Cosmic acceleration in non-flat $f(T)$ cosmology
• The $\Delta (27)$ flavor 3-3-1 model with neutral leptons
• The Gravitational Lens -- Galaxy Group Connection. II. Groups Associated with B2319+051 and B1600+434
• Coincidence Problem in YM Field Dark Energy Model
• Thermal leptogenesis with triplet Higgs boson and mass varying neutrinos
• Rossiter-McLaughlin Effect Measurements for WASP-16, WASP-25 and WASP-31
• Interacting model of new agegraphic dark energy: observational constraints and age problem
• Observational Constraints on Exponential Gravity
• Baryon Oscillations and Dark-Energy Constraints from Imaging Surveys
• SOPHIE velocimetry of Kepler transit candidates. XV. KOI-614b, KOI-206b, and KOI-680b: a massive warm Jupiter orbiting a G0 metallic dwarf and two highly inflated planets with a distant companion around evolved F-type stars
• Generic feature of future crossing of phantom divide in viable $f(R)$ gravity models
• Modulated Reheating and Large Non-Gaussianity in String Cosmology
• A Precise Estimate of the Radius of the Exoplanet HD 149026b from Spitzer Photometry
• Statefinder Diagnostic for Dilaton Dark Energy
• Generalized second law of thermodynamics for a phantom energy accreting BTZ black hole
• Model-independent measurement of cosmic curvature with the latest $H(z)$ and SNe Ia data: A comprehensive investigation
• Observational Constraints to Ricci Dark Energy Model by Using: SN, BAO, OHD, fgas Data Sets
• Testing models of supermassive black hole seed formation through gravity waves
• The D_4 flavor symmery in 3-3-1 model with neutral leptons
• Probing Dynamics of Dark Energy with Supernova, Galaxy Clustering and the Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations
• Observational Constraints on Silent Quartessence
• Interacting entropy-corrected new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe
• Inflationary potentials yielding constant scalar perturbation spectral indices
• Cosmological reconstruction of $f(T,\mathcal{T})$ Gravity
• KOI-200b and KOI-889b: two transiting exoplanets detected and characterized with Kepler, SOPHIE and HARPS-N
• A Millimetre Survey of Starburst Dominated Ultraluminous Infrared Galaxies at z~2
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• Anisotropic Universe Models in Brans-Dicke Theory
• Crossing the phantom barrier with purely kinetic multiple k-essence
• Dark energy: investigation and modeling
• Cosmological bouncing scenarios in symmetric teleparallel gravity
• Complete Set of Homogeneous Isotropic Analytic Solutions in Scalar-Tensor Cosmology with Radiation and Curvature
• Accelerating Universe scenario in anisotropic $f\left(Q\right)$ cosmology
• Generalization of Regular Black Holes in General Relativity to $f(R)$ Gravity
• Emergent Universe from Scale Invariant Two Measures Theory
• Modified gravity for surveys
• Scalar Field Dark Energy Perturbations and their Scale Dependence
• Plane Symmetric Cosmological Model with Quark and Strange Quark Matter in f(R,T) Theory of Gravity
• Non-vacuum Solutions of Bianchi Type VI_0 Universe in f(R) Gravity
• Mass bounds for compact spherically symmetric objects in generalized gravity theories
• Holographic Ricci dark energy in Randall-Sundrum braneworld: Avoidance of big rip and steady state future
• Mapping the allowed parameter space for decaying dark matter models
• Exploring stable models in $f(R;T;R_{\mu \nu }{T}^{\mu \nu })$ gravity
• Study of Gravastars in Rastall Gravity
• The nonlinear matter power spectrum
• Late Time Neutrino Masses, the LSND Experiment and the Cosmic Microwave Background
• Performance of the AMS-02 Transition Radiation Detector
• Sandage-Loeb test for the new agegraphic and Ricci dark energy models
• Anisotropic brane gravity with a confining potential
• Features of galactic halo in a brane world model and observational constraints
• Out of the Swampland with Multifield Quintessence?
• Nariai black holes with quintessence
• Planck intermediate results. XXVII. High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel-SPIRE
• New agegraphic dark energy as a rolling tachyon
• Realizing Scale-invariant Density Perturbations in Low-energy Effective String Theory
• The K2-ESPRINT Project V: a short-period giant planet orbiting a subgiant star
• Kepler Eclipsing Binaries with $\delta$ Scuti/$\gamma$ Doradus Pulsating Components 1: KIC 9851944
• Dark-matter decays and Milky Way satellite galaxies
• Gravitationally induced adiabatic particle production: From Big Bang to de Sitter
• Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in non-flat universe
• Precision of Inflaton Potential Reconstruction from CMB Using the General Slow-Roll Approximation
• Antiproton fluxes from light neutralinos
• Neutrino mixing with non-zero ${\theta }_{13}$ and CP violation in the 3-3-1 model based on $A_4$ flavor symmetry
• Dark energy model with variable $q$ and $\omega$ in LRS Bianchi-II space-time
• Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
• Warm Anisotropic Inflationary Universe Model
• The transient acceleration from time-dependent interacting dark energy models
• Light Element Signatures of Sterile Neutrinos and Cosmological Lepton Numbers
• New Interaction between Dark Energy and Dark Matter Changes Sign during Cosmological Evolution
• Shedding Light on Dark Matter: A Faraday Rotation Experiment to Limit a Dark Magnetic Moment
• Quantum FRW cosmological solutions in the presence of Chaplygin gas and perfect fluid
• Vector modes generated by primordial density fluctuations
• Pressure Parametrization of Dark Energy: First and Second-Order Constraints with Latest Cosmological Data
• Constraints on Kinematic Model from Recent Cosmic Observations: SN Ia, BAO and Observational Hubble Data
• Power-law solutions in $f(T)$ gravity
• Primordial Density Perturbation in Effective Loop Quantum Cosmology
• Cosmological neutrinos
• Consequences of energy conservation violation: Late time solutions of $\Lambda (T)CDM$ subclass of $f(R,T)$ gravity using dynamical system approach
• Large scale structure in the HI Parkes All-Sky Survey: Filling the Voids with HI galaxies?
• Addressing $H_0$ tension with emergent dark radiation in unitary gravity
• Toward More Realistic Forecasting of Dark Energy Constraints from Galaxy Redshift Surveys
• Will there be again a transition from acceleration to deceleration in course of the dark energy evolution of the universe?
• Cosmic Perturbations Through the Cyclic Ages
• Age constraints on the cosmic equation of state
• Anisotropic cosmological solutions in massive vector theories
• Accelerated Universes from type IIA Compactifications
• Eddington-Born-Infeld cosmology: a cosmographic approach, a tale of doomsdays and the fate of bound structures
• Excursion Set Halo Mass Function and Bias in a Stochastic Barrier Model of Ellipsoidal Collapse
• What is parameterized $Om(z)$ diagnostics telling us in light of recent observations?
• The Cosmological Mean Density and its Local Variations Probed by Peculiar Velocities
• Testing cosmic opacity from SNe Ia and Hubble parameter through three cosmological-model-independent methods
• Hubble Space Telescope Observations of Nine High-Redshift ESSENCE Supernovae
• Constraining warm dark matter with cosmic shear power spectra
• Cosmic age problem revisited in the holographic dark energy model
• Dark Matter in the Coming Decade: Complementary Paths to Discovery and Beyond
• Analytic rotating black hole solutions in $N$-dimensional $f(T)$ gravity
• Redshift Accuracy Requirements for Future Supernova and Number Count Surveys
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• Screening of cosmological constant for De Sitter Universe in non-local gravity, phantom-divide crossing and finite-time future singularities
• A lower mass for the exoplanet WASP-21b
• Stringy Dark Energy Model with Cold Dark Matter
• Bulk viscous embedded hybrid dark energy models
• Refined architecture of the WASP-8 system: a cautionary tale for traditional Rossiter-McLaughlin analysis
• WASP-117b: a 10-day-period Saturn in an eccentric and misaligned orbit
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• Reconstruction Procedure in Nonlocal Cosmological Models
• Top flavour violating decays in general supersymmetric models
• A Long-Period Totally Eclipsing Binary Star at the Turnoff of the Open Cluster NGC 6819 Discovered with Kepler
• Hidden past of dark energy cosmological models
• Nonparametric reconstruction of the cosmic expansion with local regression smoothing and simulation extrapolation
• Accelerating dark energy models with anisotropic fluid in Bianchi type-$V{I}_0$ space-time
• The Majorana neutrino masses, neutrinoless double beta decay and nuclear matrix elements
• Using Ultra Long Period Cepheids to Extend the Cosmic Distance Ladder to 100 Mpc and Beyond
• Neutralino Relic Density in a Supersymmetric U(1)' Model
• Energy conditions in $f(T)$ gravity with non-minimal torsion-matter coupling
• Can extra dimensional effects replace dark matter ?
• A Novel Method to Photometrically Constrain Orbital Eccentricities: Multibody Asterodensity Profiling (MAP)
• Exact relativistic beta decay endpoint spectrum
• Constraints on SUSY Seesaw Parameters from Leptogenesis and Lepton Flavor Violation
• New accelerating solutions in late-time cosmology
• Future Oscillations around Phantom Divide in f(R) Gravity
• How unitary cosmology generalizes thermodynamics and solves the inflationary entropy problem
• Candidate Disk Wide Binaries in the Sloan Digital Sky Survey
• Interacting new generalized Chaplygin gas
• Unified Dark Matter models with fast transition
• An analytic investigation of the scatter in the integrated X-ray properties of galaxy groups and clusters
• Dark radiation and dark matter coupled to holographic Ricci dark energy
• FLRW cosmological models with quark and strange quark matters in f(R,T) gravity
• Superadiabatic-type magnetic amplification in conventional cosmology
• Relativistic Interpretation of Newtonian Simulations for Cosmic Structure Formation
• Phantom-Like Behavior in $f(R)$-Gravity
• Robust sampling for weak lensing and clustering analyses with the Dark Energy Survey
• Coupled Quintessence and Phantom Based On a Dilaton
• New "Bigs" in cosmology
• Energy Conditions in $f(G)$ Modified Gravity with Non-minimal Coupling to Matter
• The Age and Distance of the Kepler Open Cluster NGC 6811 from an Eclipsing Binary, Turnoff Star Pulsation, and Giant Asteroseismology
• Statefinder hierarchy model for the Barrow holographic dark energy
• Modified Holographic Dark Energy
• Cosmological Solutions of a Nonlocal Model with a Perfect Fluid
• Probing modified gravity theories with multiple measurements of high-redshift quasars
• Warm inflation on the brane
• 3-loop Yang-Mills Condensate Dark Energy Model And Its Cosmological Constraints
• Inflation parameters from Gauss-Bonnet braneworld
• Possible antigravity regions in $F(R)$ theory?
• Tension in the Recent Type Ia Supernovae Datasets
• Measuring growth index in a universe with massive neutrinos: A revisit of the general relativity test with the latest observations
• Non-zero U_{e3} and TeV-Leptogenesis through A_4 symmetry breaking
• Cosmological dynamics of fourth order gravity: A compact view
• Stability of Anisotropic Stellar Filaments
• Revisiting the Cosmological Constraints on the Interacting Dark Energy Models
• Reconstruction of f(T) gravity according to holographic dark energy
• $f(R)$ gravity theories in the Palatini Formalism constrained from strong lensing
• GaBoDS: The Garching-Bonn Deep Survey: VII. Probing galaxy bias using weak gravitational lensing
• An effective description of dark matter and dark energy in the mildly non-linear regime
• Joint Analysis of Gravitational Lensing, Clustering and Abundance: Toward the Unification of Large-Scale Structure Analysis
• On Anisotropic Dark Energy
• Non-minimal Maxwell-Modified Gauss-Bonnet Cosmologies: Inflation and Dark Energy
• Anthropic predictions for neutrino masses
• Relic density of neutralino dark matter in the MSSM with CP violation
• Holography and the scale-invariance of density fluctuations
• New Exact Spherically Symmetric Solutions in $f(R,\varphi ,X)$ gravity by Noether's symmetry approach
• A novel teleparallel dark energy model
• A note on electromagnetic and gravitational perturbations of the Bardeen de Sitter black hole: quasinormal modes and greybody factors
• Evidence for Early Filamentary Accretion from the Andromeda Galaxy's Thin Plane of Satellites
• The Cosmic Microwave Background for Pedestrians: A Review for Particle and Nuclear Physicists
• A First Glimpse of String Theory in the Sky?
• Growth of matter perturbations in clustered holographic dark energy cosmologies
• Scaling solutions in scalar-tensor cosmologies
• Toward a Unified Description of Dark Energy and Dark Matter from the Abnormally Weighting Energy Hypothesis
• Doubly special relativity in de Sitter spacetime
• How Late can the Dark Matter form in our universe?
• Transition Redshift: New constraints from parametric and nonparametric methods
• Halo stochasticity in global clustering analysis
• Cosmology in scalar-vector-tensor theories
• Exploring the Systematic Uncertainties of Type Ia Supernovae as Cosmological Probes
• Stability analysis of anisotropic Bianchi type-I cosmological model in teleparallel gravity
• New Agegraphic Dark Energy in $f(R)$ Gravity
• Narrowing Constraints with Type Ia Supernovae: Converging on a Cosmological Constant
• Transitioning Universe with hybrid scalar field in Bianchi I space-time
• Dark Matter and The Anthropic Principle
• Redshift space 21 cm power spectra from reionization
• Probing Dark Energy in The scope of Bianchi type I Spacetime
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• The Integrated Sachs-Wolfe Effect in Interacting Dark Energy Models
• Some remarks about non-minimally coupled scalar field models
• Dark energy and dark matter from cosmological observations
• Phantom cosmology in an Extended Theory of Gravity
• Testing Fractional Action Cosmology
• Interacting new agegraphic viscous dark energy with varying $G$
• Regularizing cosmological singularities by varying physical constants
• Photon Geodesics in FRW Cosmologies
• The holographic induced gravity model with a Ricci dark energy: smoothing the little rip and big rip through Gauss-Bonnet effects?
• Unified Dark Matter scalar field models with fast transition
• Mechanics and Newton-Cartan-Like Gravity on the Newton-Hooke Space-time
• A closer look at interacting dark energy with statefinder hierarchy and growth rate of structure
• Cosmological Parameters from the SDSS DR5 Velocity Dispersion Function of Early-Type Galaxies through Radio-Selected Lens Statistics
• Cosmic acceleration and crossing of $\omega =-1$ in non-minimal modified Gauss-Bonnet gravity
• Trapped Quintessential Inflation
• New Constraints on Macroscopic Compact Objects as a Dark Matter Candidate from Gravitational Lensing of Type Ia Supernovae
• Fine Tuning Free Paradigm of Two Measures Theory: K-Essence, Absence of Initial Singularity of the Curvature and Inflation with Graceful Exit to Zero Cosmological Constant State
• The UV-optical colours of brightest cluster galaxies in optically and X-ray selected clusters
• From Primordial Quantum Fluctuations to the Anisotropies of the Cosmic Microwave Background Radiation
• Dark Energy from graviton-mediated interactions in the QCD vacuum
• Tight constraints on the existence of additional planets around HD 189733
• Bounce cosmology in $f(\mathcal{R})$ gravity
• Systematic Parameter Space Search of Extended Quark-Lepton Complementarity
• Testing Mass Varying Neutrino With Short Gamma Ray Burst
• Detecting neutrino mass difference with cosmology
• The Very Short Period M Dwarf Binary SDSS J001641-000925
• Cosmic Constraint on Ricci Dark Energy Model
• Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
• Spitzer observations of a gravitationally lensed quasar, QSO 2237+0305
• Exploring compressed supersymmetry with same-sign top quarks at the Large Hadron Collider
• An upper limit to polarized submillimetre emission in Arp 220
• Implications of a new temperature scale for halo dwarfs on LiBeB and chemical evolution
• Can Holographic dark energy models fit the observational data?
• Susskind's Challenge to the Hartle-Hawking No-Boundary Proposal and Possible Resolutions
• Cosmic Behavior, Statefinder Diagnostic and $w-w^{\prime }$ Analysis for Interacting NADE model in Non-flat Universe
• Construction of Exact Solutions in Two-Fields Models and the Crossing of the Cosmological Constant Barrier
• Tachyon-Chaplygin inflationary universe model
• Statefinder Parameters for Interacting Phantom Energy with Dark Matter
• Remarks on Dynamical Dark Energy Measured by the Conformal Age of the Universe
• A Generalized Interacting Tsallis Holographic Dark Energy Model and its thermodynamic implications
• Dynamical Mass of the M8+M8 Binary 2MASS J22062280-2047058AB
• Composite dark energy: cosmon models with running cosmological term and gravitational coupling
• Holographic dark energy in a non-flat universe with Granda-Oliveros cut-off
• Model selection and constraints from Holographic dark energy scenarios
• $\Lambda$-CDM Universe: A Phenomenological Approach With Many Possibilities
• Neutrino Mixing with Non-Zero ${\theta }_{13}$ and CP Violation in the 3-3-1 Model Based on $S_4$ Flavor Symmetry
• Third order perturbations of a zero-pressure cosmological medium: Pure general relativistic nonlinear effects
• Quasinormal modes and absorption cross sections of Born-Infeld-de Sitter black holes
• IceHEP High Energy Physics at the South Pole
• Gravitational Waves in Viable f(R) Models
• The running-mass inflation model and WMAP
• Fitting Non-Minimally Coupled Scalar Models to Gold SnIa Dataset
• Dynamical Evolution of Interacting Modified Chaplygin Gas
• QCD ghost f(T)-gravity model
• Joint cosmological parameters forecast from CFHTLS-cosmic shear and CMB data
• D-term chaotic inflation in supergravity
• Leptogenesis and dark matter unified in a non-SUSY model for neutrino masses
• Spatially Hyperbolic Gravitating Sources in $\Lambda$-Dominated Era
• Intermediate inflation on the brane
• Power-Law Entropy Corrected Ricci Dark Energy and Dynamics of Scalar Fields
• Reconstructing a String-Inspired Quintom Model of Dark Energy
• Dark matter search by exclusive studies of X-rays following WIMPs nuclear interactions
• Comparison of Recent SnIa datasets
• Matter Power Spectrum for the Generalized Chaplygin Gas Model: The Newtonian Approach
• Coupling Quintessence to Inflation in Supergravity
• Dynamics of holographic vacuum energy in the DGP model
• Cosmological Constraints from Hubble parameter $H(z)$ and SN Ia observations
• Virialization of cosmological structures in models with time varying equation of state
• Observational constraints on cosmic neutrinos and dark energy revisited
• Extended Born-Infeld Dynamics and Cosmology
• Couplings between holographic dark energy and dark matter
• Affine parameterization of the dark sector: costraints from WMAP5 and SDSS
• Neutrino flavor ratios as diagnostic of solar WIMP annihilation
• Constraints on Dark Energy Models Including Gamma Ray Bursts
• Can high-redshift Hubble diagrams rule out the standard model of cosmology in the context of cosmographic method?
• Cosmology With Low-Redshift Observations: No Signal For New Physics
• Chaotic universe model: Lotka-Volterra dynamics of the universe evolution
• Observational Constraints on Planet Nine: Cassini Range Observations
• A Prescription for Galaxy Biasing Evolution as a Nuisance Parameter
• Two-fluid atmosphere from decelerating to accelerating FRW dark energy models
• Generalized holographic dark energy model described at the Hubble length
• Observational Constraints of Modified Chaplygin Gas in Loop Quantum Cosmology
• Statefinder diagnostic and $w-w^{\prime }$ analysis for interacting polytropic gas dark energy model
• The full Fisher matrix for galaxy surveys
• Non-Gaussianity in Large Scale Structure and Minkowski Functionals
• Radii of Rapidly-Rotating Stars, with Application to Transiting-Planet Hosts
• Mutated Hilltop Inflation : A Natural Choice for Early Universe
• Baryon Acoustic Oscillations and Dynamical Dark Energy
• Quintessence and the Transition to an Accelerating Universe
• Detection of period variations in extrasolar transiting planet OGLE-TR-111b
• A Measurement of Arcminute Anisotropy in the Cosmic Microwave Background with the Sunyaev-Zel'dovich Array
• Chaplygin inflation on the brane
• Cosmological constraints on general, single field inflation
• The Transit Light Curve Project. IV. Five Transits of the Exoplanet OGLE-TR-10b
• Tightening geometric and dynamical constraints on dark energy and gravity: galaxy clustering, intrinsic alignment and kinetic Sunyaev-Zel'dovich effect
• Study Of Tachyon Dynamics For Broad Classes of Potentials
• Detailed study of geodesics in the Kerr-Newman-(A)dS spactime and the rotating charged black hole spacetime in $f(R)$ gravity
• Cosmic opacity: cosmological-model-independent tests from gravitational waves and Type Ia Supernova
• Holographic dark energy in Brans-Dicke cosmology with Granda-Oliveros cut-off
• Neutrino Mixings and Leptonic CP Violation from CKM Matrix and Majorana Phases
• Can Old Galaxies at High Redshifts and Baryon Acoustic Oscillations Constrain H_0?
• Do We Have Evidence for New Physics in the Sky?
• The top squark-mediated annihilation scenario and direct detection of dark matter in compressed supersymmetry
• Exact nonlinear inhomogeneities in $\Lambda$CDM cosmology
• Modified Chaplygin Traversable Wormholes
• KIC 1571511B: A Benchmark Low-Mass Star In An Eclipsing Binary System In The Kepler Field
• The SUGRA Quintessence Model Coupled to the MSSM
• Cosmological Constant Problems and Renormalization Group
• Agegraphic dark energy: growth index and cosmological implications
• Forecasts of non-Gaussian parameter spaces using Box-Cox transformations
• Tsallis holographic dark energy in Fractal Universe
• The w = -1 crossing of the quintom model with slowly-varying potentials
• Dynamics of perfect fluid Unified Dark Energy models
• FLRW cosmology with EDSFD parametrization
• Modified holographic dark energy in DGP brane world
• Cosmological tests of sudden future singularities
• Thermodynamic properties of modified gravity theories
• Bianchi Type $I$ Cosmology in $f(R,T)$ Gravity
• How Does Radio AGN Feedback Feed Back?
• New Generalizations of Cosmography Inspired by the Pade Approximant
• Accretion of Phantom Energy and Generalized Second Law of Thermodynamics for Einstein-Maxwell-Gauss-Bonnet Black Hole
• Crossing of $\omega =-1$ with Tachyon and Non-minimal Derivative Coupling
• On cosmological signatures of baryons-dark energy elastic couplings
• Reconstruction of modified gravity with ghost dark energy models
• Confronting the Hubble Diagram of Gamma-Ray Bursts with Cardassian Cosmology
• An Accelerating Cosmological Model from a Parametrization of Hubble Parameter
• Direction Dependent Non-gaussianity in High-z Supernova Data
• Transiting exoplanets from the CoRoT space mission XXI. CoRoT-19b: A low density planet orbiting an old inactive F9V-star
• Tsallis cosmology and its applications in dark matter physics with focus on IceCube high-energy neutrino data
• A Light Echo from Type Ia Supernova 1995E?
• Neutrino masses from clustering of red and blue galaxies: a test of astrophysical uncertainties
• Correction to Lagrangian for Bouncing Cosmologies in $f(Q)$ Gravity
• Cosmic Mimicry: Is LCDM a Braneworld in Disguise ?
• Dark Matter and Dark Energy from a single scalar field and CMB data
• Exotic Low Density Fermion States in the Two Measures Field Theory: Neutrino Dark Energy
• D6 Family Symmetry and Cold Dark Matter at LHC
• Measuring the reionization optical depth without large-scale CMB polarization
• Geodesic Deviation Equation in $f(R,T)$ Gravity
• Modeling Kepler Eclipsing Binaries: Homogeneous Inference of Orbital & Stellar Properties
• Observing the metal-poor solar neighbourhood: a comparison of galactic chemical evolution predictions
• Estimating the masses of extra-solar planets
• The solution of the cosmological constant problem from the inhomogeneous equation of state - a hint from modified gravity?
• Warm-Chaplygin inflationary universe model
• Cold Dark Matter in non-Standard Cosmologies, PAMELA, ATIC and Fermi LAT
• On the accuracy of slow-roll inflation given current observational constraints
• Post-Newtonian Approximation of Teleparallel Gravity Coupled with a Scalar Field
• A Comparison of Cosmological Models Using Strong Gravitational Lensing Galaxies
• Cosmological consequences and statefinder diagnosis of a non-interacting generalized Chaplygin gas in $f(R,T)$ gravity
• Testing for dynamical dark energy models with redshift-space distortions
• Dispersive Light Propagation at Cosmological Distances: Matter Effects
• Statefinder diagnosis and the interacting ghost model of dark energy
• Local primordial non-Gaussianity from the large-scale clustering of photometric DESI luminous red galaxies
• Ground-based multisite observations of two transits of HD 80606b
• Testing the DGP model with gravitational lensing statistics
• CoRoT 101186644: A transiting low-mass dense M-dwarf on an eccentric 20.7-day period orbit around a late F-star
• Thermal leptogenesis in a TeV scale model for neutrino masses
• Constraining $H_0$ from Sunyaev-Zel'dovich effect, Galaxy Clusters X-ray data, and Baryon Oscillations
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• WMAP 5-year constraints on lepton asymmetry and radiation energy density: Implications for Planck
• Long range correlation in cosmic microwave background radiation
• Thermodynamics of the viscous $f(T,B)$ gravity in the new agegraphic dark energy model
• Effects of Anisotropy on the Sign-Changeable Interacting Tsallis Holographic Dark Energy
• Phase space analysis of quintessence fields trapped in a Randall-Sundrum braneworld: a refined study
• Phantom-like behaviour in a brane-world model with curvature effects
• Cosmological implications of an interacting model of dark matter \& dark energy
• Why Newton's gravity is practically reliable in the large-scale cosmological simulations
• Tolman IV fluid sphere in f(R, T) gravity
• Wormhole on the Brane with Ordinary Matter: The Broader View
• Probing Inflation and Dark Energy with Current Cosmological Observations
• Extending the Coyote emulator to dark energy models with standard $w_0$-$w_a$ parametrization of the equation of state
• Supernova Constraints on Models of Neutrino Dark Energy
• Thermodynamics in Closed Universe with Entropy Corrections
• Dark energy reconstruction based on the PADE approximation; an expansion around the $\Lambda$CDM
• Attractor behaviour of $f(T)$ modified gravity and the cosmic acceleration
• Saez-Ballester gravity in Kantowski-Sachs Universe: a new reconstruction paradigm for Barrow Holographic Dark Energy
• Cosmological viability conditions for $f(T)$ dark energy models
• Constraints on Tsallis Cosmology from Big Bang Nucleosynthesis and the Relic Abundance of Cold Dark Matter Particles
• Dark Matter
• Quintessential Kination and Thermal Production of Gravitinos and Axinos
• Reconstructing the potentials for the quintessence and tachyon dark energy, from the holographic principle
• Statefinder diagnosis for holographic dark energy in the DGP braneworld
• Temperature at Horizon in de Sitter Spacetime
• Domain wall solution in $F(R)$ gravity and variation of the fine structure constant
• Inflation in Loop Quantum Cosmology
• Modified Chaplygin Gas Cosmology with Bulk Viscosity
• Is thermodynamics of the universe bounded by the event horizon a Bekenstein system?
• Fourier Phase Analysis of SDSS Galaxies
• Observational constraint on the interacting dark energy models including the Sandage-Loeb test
• Zeta Function Methods and Quantum Fluctuations
• Evidence for cosmic neutrino background form CMB circular polarization
• Two Component Model of Dark Energy
• The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity
• Matter Power Spectra in Viable $f(R)$ Gravity Models with Massive Neutrinos
• A comprehensive investigation on the slowing down of cosmic acceleration
• Galactic rotation curves inspired by a noncommutative-geometry background
• Dynamical system analysis in teleparallel gravity with boundary term
• Did Boomerang hit MOND?
• Tradeoff between Smoother and Sooner "Little Rip"
• Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise
• Quasinormal modes of scalar and Dirac perturbations of Bardeen de-Sitter black holes
• Dark energy interacting with two fluids
• On extended sign-changeable interactions in the dark sector
• Inflation from D3-brane motion in the background of D5-branes
• A direct link between neutrinoless double beta decay and leptogenesis in a seesaw model with $S_4$ symmetry
• The Most Massive Black Holes in the Universe: Effects of Mergers in Massive Galaxy Clusters
• Phase space analysis of bulk viscous matter dominated universe
• Direct Dark Matter Searches
• Cosmographic analysis of a closed bouncing universe with the varying cosmological constant in $f(R,T)$ gravity
• The cosmic web for density perturbations of various scales
• Thermodynamical aspects of relativistic hydrodynamics in f(R,G) gravity
• Reconstructing interacting new agegraphic polytropic gas model in non-flat FRW universe
• Dark matter in the supersymmetric radiative seesaw model with an anomalous U(1) symmetry
• Dark Energy Interacting with Dark Matter in Classical Einstein and Loop Quantum Cosmology
• Luminosity distance-redshift relation for the LTB solution near the center
• Oscillating universe in massive gravity
• The distinctions between $\Lambda$CDM and $f(T)$ gravity according Noether symmetry
• Fractional-order derivatives in cosmological models of accelerated expansion
• Generalised nonminimally gravity-matter coupled theory
• Galactic rotation curves and brane world models
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• Nonlinear corrections to the cosmological matter power spectrum and scale-dependent galaxy bias: implications for parameter estimation
• Cosmological Constraints on Variable Warm Dark Matter
• Observations of the WASP-2 System by the APOSTLE Program
• Constraints on Neutrino Mass and Light Degrees of Freedom in Extended Cosmological Parameter Spaces
• Noether symmetries and boundary terms in extended Teleparallel gravity cosmology
• Bouncing universe with the non-minimally coupled scaler field and its reconstructing
• High-energetic Cosmic Antiprotons from Kaluza-Klein Dark Matter
• The conformal status of $\omega =-3/2$ Brans-Dicke cosmology
• Trapped Quintessential Inflation in the context of Flux Compactifications
• Geometrical Constraints on Dark Energy
• Effects of early dark energy on strong cluster lensing
• Through the Looking Glass: Why the "Cosmic Horizon" is not a horizon
• Light neutralinos at LHC in cosmologically-inspired scenarios: new benchmarks in the search for supersymmetry
• Quasinormal modes of dilaton-de Sitter black holes: scalar perturbations
• Probing the cosmic opacity from Future Gravitational Wave Standard Sirens
• LHC Phenomenology and Cosmology of String-Inspired Intersecting D-Brane Models
• On The Direct Detection of Dark Matter- Exploring all the signatures of the neutralino-nucleus interaction
• Expansion history and f(R) modified gravity
• Moduli Fields as Quintessence and the Chameleon
• Variable G correction to statefinder parameters of dark energy
• The Lack of Structural and Dynamical Evolution of Elliptical Galaxies since z ~ 1.5: Clues from Self-Consistent Hydrodynamical Simulations
• Dynamical Dark Energy Implies a Coupled Dark Sector: Insights from DESI DR2 via a Data-Driven Approach
• Evolution of spherical overdensities in holographic dark energy models
• Anisotropic k-essence cosmologies
• Role of Non-conserved Gravity Theory and Electric Charge in Constructing Complexity-free Stellar Models: A Novel Approach under Non-minimal Coupling
• Reconstructing generalized ghost condensate model with dynamical dark energy parametrizations and observational datasets
• An Integrated Analysis of Radial Velocities in Planet Searches
• Holes in the static Einstein universe and the model of the cosmological voids
• Using the cluster mass function from weak lensing to constrain neutrino masses
• Dark matter, dark energy, and dark radiation coupled with a transversal interaction
• Interacting Dark Energy in Hořava-Lifshitz Cosmology
• The Accelerated Acceleration of the Universe
• Ghost dark energy in $f(R)$ model of gravity
• Dynamical Systems analysis of an interacting dark energy model in the Brane Scenario
• A Realistic Particle Physics Dark Energy Model
• Second-Order Corrections to the Power Spectrum in the Slow-Roll Expansion with a Time-Dependent Sound Speed
• Nonthermal production of baryon and dark matter
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Interacting viscous ghost tachyon, K-essence and dilaton scalar field models of dark energy
• Cosmological neutrino bounds for non-cosmologists
• The stellar populations of the bluest low surface brightness galaxies
• Boundary Inflation and the WMAP Data
• Exploring the Sharma-Mittal HDE models with different diagnostic tools
• Single Field Inflation models allowed and ruled out by the three years WMAP data
• Spin-orbit alignments for Three Transiting Hot Jupiters: WASP-103b, WASP-87b, & WASP-66b
• Effects of ghost dark energy perturbations on the evolution of spherical overdensities
• Black hole and holographic dark energy
• Observational constraints on phantom power-law cosmology
• Higher-Order Angular Galaxy Correlations in the SDSS: Redshift and Color Dependence of non-Linear Bias
• Photometric Follow-up Observations of the Transiting Neptune-Mass Planet GJ 436b
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• Evolution of superclusters in the cosmic web
• Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying $\beta$ and different light-curve fitters
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• Thermal radiation from Lorentzian traversable wormholes
• Holographic Dark Energy from a Modified GBIG Scenario
• Kantowski-Sachs Universe Models in $f(T)$ Theory of Gravity
• On dark matter - dark radiation interaction and cosmic reionization
• A model independent approach to the study of $f(R)$ cosmologies with expansion histories close to $\Lambda$CDM
• The Influence of Galaxy Formation Physics on Weak Lensing Tests of General Relativity
• Inducing the cosmological constant from five-dimensional Weyl space
• Constraints on the solid dark universe model
• Scalar-field theory of dark matter
• Dark energy parameterizations and their effect on dark halos
• Interacting Two-Fluid Viscous Dark Energy Models In Non-Flat Universe
• Nonlinear Spinor Fields in Bianchi type-I spacetime: Problems and Possibilities
• Cosmological Models and Latest Observational Data
• Measuring the geometry of the Universe in the presence of isocurvature modes
• Noether Gauge Symmetry of Modified Teleparallel Gravity Minimally Coupled with a Canonical Scalar Field
• Model-independent determination of the cosmic expansion rate. I. Application to type-Ia supernovae
• Absolute parameters for AI Phoenicis using WASP photometry
• Generalized Chaplygin gas model: Cosmological consequences and statefinder diagnosis
• A Cyclic Universe With Varying Cosmological Constant in $f(R,T)$ gravity
• Observational constraints on decaying vacuum dark energy model
• Equations of State in the Brans-Dicke cosmology
• The dynamical viability of scalar-tensor gravity theories
• Cosmological models in $f(T,\mathcal{T})$ gravity and the dynamical system analysis
• $B_s-\overline{B_s}$ mixing, B decays and R-parity violating supersymmetry
• Dark Energy and the MSSM
• Reconstruction of new holographic scalar field models of dark energy in Brans-Dicke Universe
• Observational Constraints on Dynamical Dark Energy Models
• Cosmological Evolution Across Phantom Crossing and the Nature of the Horizon
• Accelerating bianchi type dark energy cosmological model with cosmic string in f(T) Gravity
• Scalar-Tensor Teleparallel Gravity With Boundary Term by Noether Symmetries
• Strong gravitational lensing constraints on holographic dark energy
• Cosmology with nonminimal kinetic coupling and a Higgs-like potential
• Reconstruction of interaction rate in Holographic dark energy model with Hubble horizon as the infrared cut-off
• New general parametrization of quintessence fields and its observational constraints
• Radiative corrections to stoponium annihilation decays
• Generalized interacting Barrow Holographic Dark Energy: cosmological predictions and thermodynamic considerations
• Cosmology of non-minimal derivative coupling to gravity in Palatini formalism and its chaotic inflation
• Oxidised cosmic acceleration
• Neutrino masses and mixings in the baryon triality constrained minimal supersymmetric standard model
• New holographic dark energy model with non-linear interaction
• Statefinder Analysis of Symmetric Teleparallel Cosmology
• Does fractal Universe describe a complete cosmic scenario?
• Dark energy models toward observational tests and data
• Modeling holographic dark energy with particle and future horizons
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• Illuminating Dark Energy with Cosmic Shear
• Ricci dark energy in bumblebee gravity model
• DM haloes in the fifth-force cosmology
• Clues on Regularity in the Structure and Kinematics of Elliptical Galaxies from Self-consistent Hydrodynamical Simulations: the Dynamical Fundamental Plane
• Second order perturbations of a zero-pressure cosmological medium: Proofs of the relativistic-Newtonian correspondence
• Two-Fluid Dark Energy Models in Bianchi Type-III Universe with Variable Deceleration Parameter
• Thermodynamics and stability of $f(T,B)$ gravity with viscous fluid by observational constraints
• Stability of domain walls in models with asymmetric potentials
• Geodesic Structure of the Quantum-Corrected Schwarzschild Black Hole Surrounded by Quintessence
• The generalized second law for the interacting generalized Chaplygin gas model
• Tangled magnetic fields and CMBR signal from reionization epoch
• Mass-Varying Neutrinos from a Variable Cosmological Constant
• Stability and interacting $f(T,\mathcal{T})$ gravity with modified Chaplygin gas
• Neutrino mass bounds from cosmology
• Relativistic-Newtonian correspondence of the zero-pressure but weakly nonlinear cosmology
• String Inspired Quintom Model with Non-minimally Coupled Modified Gravity
• Observing Dark Matter via the Gyromagnetic Faraday Effect
• Can we test Dark Energy with Running Fundamental Constants ?
• Cosmic microwave background constraints on dark energy dynamics: analysis beyond the power spectrum
• Review Article: Physics and Monte Carlo Techniques as Relevant to Cryogenic, Phonon and Ionization Readout of CDMS Radiation-Detectors
• Stochastic Quintessence
• Can MSSM Particle be the Inflaton?
• A new light on the darkest corner of the landscape
• Joint constraints on the lepton asymmetry of the Universe and neutrino mass from the Wilkinson Microwave Anisotropy Probe
• Characterization of the four new transiting planets KOI-188b, KOI-195b, KOI-192b, and KOI-830b
• Thermodynamics of Schwarzschild black hole surrounded by quintessence in gravity's rainbow
• Holographic kinetic k-essence model
• The Influence of Free Quintessence on Gravitational Frequency Shift and Deflection of Light with 4D momentum
• Viscous Generalized Chaplygin Gas as a Unified Dark Fluid: Including Perturbation of Bulk Viscosity
• Cosmological Parameters from the QUaD CMB polarization experiment
• Ground-based transit observations of the super-Earth GJ 1214b
• Modified GBIG Scenario as an Alternative for Dark Energy
• Cluster counts: calibration issue or new physics?
• Spherical collapse model and cluster number counts in power law $f(T)$ gravity
• An optimal estimator for the CMB-LSS angular power spectrum and its application to WMAP and NVSS data
• Will black holes eventually engulf the universe?
• Constraints on the dark matter and dark energy interactions from weak lensing bispectrum tomography
• Dynamical systems of modified Gauss-Bonnet gravity: cosmological implications
• Accelerating Dark Energy Cosmological Model in Two Fluid with Hybrid Scale Factor
• Constraints on oscillating dark energy models
• Growth of structure in interacting vacuum cosmologies
• Reconstruction of an Observationally Constrained $f(R,T)$ gravity model
• Interacting entropy-corrected new agegraphic dark energy in non-flat universe
• Nonlinear Period-Luminosity Relation for the Large Magellanic Cloud Cepheids: Myths and Truths
• Second-order matter density perturbations and skewness in scalar-tensor modified gravity models
• Optical characterization of WISE selected blazar candidates
• Cosmic acceleration and extra dimensions: constraints on modifications of the Friedmann equation
• Cosmography and large scale structure by f(R) gravity: new results
• Nonparametric reconstruction of the Om diagnostic to test LCDM
• Extended percolation analysis of the cosmic web
• Thermodynamic Phase Transition and global stability of the Regular Hayward Black hole Surrounded by Quintessence
• Comparing holographic dark energy models with statefinder
• Noether gauge symmetry for the Bianchi type I model in f(T) gravity
• Quintessential power-law cosmology: dark energy equation of state
• Fixed points and FLRW cosmologies: Flat case
• Perturbations of ionization fractions at the cosmological recombination epoch
• Scaling ansatz, four zero Yukawa textures and large ${\theta }_{13}$
• Optical, X-ray, and $\gamma$-ray observations of the candidate transitional millisecond pulsar 4FGL J0427.8-6704
• Cosmological models with Yang-Mills fields
• Bouncing Universe and phantom crossing in Modified Gravity and its reconstruction
• Smoothed Particle Inference: A Kilo-Parametric Method for X-ray Galaxy Cluster Modeling
• A new extended quintessence
• Cosmological dark energy effects from entanglement
• Observational constraints on the dark energy density evolution
• Analyzing the Scalar Top Co-Annihilation Region at the ILC
• Characteristic Angular Scales in Cosmic Microwave Background Radiation
• Cosmology with variable parameters and effective equation of state for Dark Energy
• Dark Energy, A Cosmological Constant, and Type Ia Supernovae
• A more general interacting model of holographic dark energy
• From the Spectrum to Inflation : An Inverse Formula for the General Slow-Roll Spectrum
• A single model of interacting dark energy: generalized phantom energy or generalized Chaplygin gas
• Non-parametric reconstruction of dark energy and cosmic expansion from the Pantheon compilation of type Ia supernovae
• Anisotropic solid dark energy
• Dynamical systems analysis of phantom models
• The Mid-Infrared Period-Luminosity Relations for the Small Magellanic Cloud Cepheids Derived from Spitzer Archival Data
• Gaugessence: a dark energy model with early time radiation-like equation of state
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• 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
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering
• Anisotropic Spheres Via Embedding Approach in $f(R,\varphi ,X)$ Gravity
• On the future of Gamma-Ray Burst Cosmology
• Searching for Composite Neutrinos in the Cosmic Microwave Background
• Not a Copernican observer: biased peculiar velocity statistics in the local Universe
• Kinematic Evidence for Halo Substructure in Spiral Galaxies
• Observational signatures of a non-singular bouncing cosmology
• Orbifold Physics and de Sitter Spacetime
• Bianchi type VI1 cosmological model with wet dark fluid in scale invariant theory of gravitation
• Noether Symmetries of Some Homogeneous Universe Models in Curvature Corrected Scalar-Tensor Gravity
• A Unified Model of Phantom Energy and Dark Matter
• A Massive Field-Theoretic Model for Hodge Theory
• Halo based reconstruction of the cosmic mass density field
• Interacting modified holographic Ricci dark energy model and statefinder diagnosis in flat universe
• On the Systematic Errors of Cosmological-Scale Gravity Tests using Redshift Space Distortion: Non-linear Effects and the Halo Bias
• Tachyon-Chaplygin inflation on the brane
• Gödel-type universes in f(T) gravity
• Precision Cosmology: Successes and Challenges
• Is it possible to tell the difference between fermionic and bosonic hot dark matter?
• Steerable wavelet analysis of CMB structures alignment
• Observational constraints on the oscillating dark energy cosmologies
• A model-independent dark energy reconstruction scheme using the geometrical form of the luminosity-distance relation
• Corrected holographic dark energy with power-law entropy and Hubble Horizon cut-off in FRW Universe
• Thawing models in the presence of a generalized Chaplygin gas
• Constraining Self-Interacting Dark Matter with Dwarf Spheroidal Galaxies and High-resolution Cosmological $N$-body Simulations
• Generation of large-scale magnetic fields from inflation in teleparallelism
• Holographic dark energy with the sign-changeable interaction term
• Best values of parameters for interacting HDE with GO IR-cutoff in Brans-Dicke cosmology
• Dynamics of an Anisotropic Universe in $f(R,T)$ Theory
• Transient Crossing of Phantom divide line $w_{\Lambda }=-1$ under Gauss-Bonnet interaction
• Scintillation-only Based Pulse Shape Discrimination for Nuclear and Electron Recoils in Liquid Xenon
• Optimal ISW detection and joint likelihood for cosmological parameter estimation
• Cosmological evolution of interacting dark energy in Lorentz violation
• Attractor Solution in Coupled Yang-Mills Field Dark Energy Models
• Interacting $F(R,T)$ gravity with modified Chaplygin gas
• PeV IceCube signals and Dark Matter relic abundance in modified cosmologies
• Parametrization of K-essence and Its Kinetic Term
• First Results from a Broadband Search for Dark Photon Dark Matter in the $44$ to $52\mu$eV range with a coaxial dish antenna
• Holographic approach for dark energy - dark matter interaction in curved FLRW spacetime
• On Reconstruction of Extended Teleparallel Gravity from the Cosmological Jerk Parameter
• Asymptotic behavior of w in general quintom model
• Local Gravity Constraints and Power Law f(R) Theories
• Cosmological constraints from Radial Baryon Acoustic Oscillation measurements and Observational Hubble data
• Age of the Universe in the Cardassian Model
• Period-color and amplitude-color relations in classical Cepheid variables V: The Small Magellanic Cloud Cepheid models
• Group theoretical interpretation of the modified gravity in de Sitter space
• Consistency of LCDM with Geometric and Dynamical Probes
• The K2-ESPRINT Project II: Spectroscopic follow-up of three exoplanet systems from Campaign 1 of K2
• A dynamical system representation of generalized Rastall gravity
• Anisotropic Dark Energy Bianchi Type III Cosmological Models in Brans Dicke Theory of Gravity
• Exponential Cardassian Universe
• Clustering dark energy imprints on cosmological observables of the gravitational field
• Cosmological evolution of equation of state for dark energy in G-essence models
• Gamma Rays Bursts: A Viable Cosmological Probe?
• A solar twin in the eclipsing binary LL Aqr
• Anisotropic $k$-essence
• Analytic solutions of the geodesic equation for Reissner-Nordström-(anti-)de Sitter black holes surrounded by different kinds of regular and exotic matter fields
• Sounds of instability from generalized QCD ghost dark energy
• Matter Quantum Corrections to the Graviton Self-Energy and the Newtonian Potential
• Tension between SN and BAO: current status and future forecasts
• The classical and quantum implications of the Raychaudhuri Equation in f(T)-gravity
• Impact of Systematic Errors in Sunyaev-Zel'dovich Surveys of Galaxy Clusters
• Combined constraints on Cardassian models from supernovae, CMB and large-scale structure observations
• Dark Matter Constraints from a Cosmic Index of Refraction
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Bianchi type-I Dust Filled Accelerating Brans- Dicke Cosmology
• Big Bang Nucleosynthesis with Independent Neutrino Distribution Functions
• The luminosity-redshift relation in brane-worlds: I. Analytical results
• Neutrino mass constraints on beta decay
• Bayesian analysis of bulk viscous matter dominated universe
• Inflessence: a phenomenological model for inflationary quintessence
• Cosmological implications of interacting polytropic gas dark energy model in non-flat universe
• The clustering of baryonic matter. I: a halo-model approach
• Study of Tsallis holographic dark energy model in the framework of Fractal cosmology
• Cosmological bounds on oscillating dark energy models
• Reconstructing f(R) Gravity from a Chaplygin Scalar Field in de Sitter Spacetimes
• Self-interacting holographic dark energy
• Density preturbations in a finite scale factor singularity universe
• Using Big Bang Nucleosynthesis to Extend CMB Probes of Neutrino Physics
• Schrödinger-Wheeler-DeWitt equation in chaplygin gas FRW cosmological model
• Dark Matter at the Fermi Scale
• The minimum mass of a charged spherically symmetric object in $D$ dimensions, its implications for fundamental particles, and holography
• On Power and Complementarity of the Experimental Constraints on Seesaw Models
• Euler-Heisenberg black hole surrounded by quintessence in the background of perfect fluid dark matter: Thermodynamics, Shadows and Quasinormal modes
• Cosmography of interacting generalized QCD ghost dark energy
• Cosmic evolution in f(T) gravity theory
• Spherical collapse model in agegraphic dark energy cosmologies
• The Impact of Non-Gaussianity upon Cosmological Forecasts
• Observable Quantities in Weyl Gravity
• The luminosity-redshift relation in brane-worlds: II. Confrontation with experimental data
• A New Type of Dark Energy Model
• Mock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
• Probing dark matter models with neutrinos from the Galactic center
• Evolving dark energy equation of state and CMB/LSS cross-correlation
• A Beginner's Guide to the Theory of CMB Temperature and Polarization Power Spectra in the Line-of-Sight Formalism
• Massive scalar field quasinormal modes of a Schwarzschild black hole surrounded by quintessence
• Holographic interacting dark energy in the braneworld cosmology
• Phantom Instability of Viscous Dark Energy in Anisotropic Space-Time
• Light Sterile Neutrinos and Inflationary Freedom
• Constraints on the DGP Universe Using Observational Hubble parameter
• Extracting New Physics from the CMB
• Chaplygin gas may prevent big trip
• Age Problem in Lemaitre-Tolman-Bondi Void Models
• Cosmic Evolution in Self-Interacting Brans-Dicke Cosmology
• Cosmological Black Holes as Seeds of Voids in Galaxy Distribution
• On a possible compensation of the QCD vacuum contribution to the Dark Energy
• Regular black holes in de Sitter universe: scalar field perturbations and quasinormal modes
• Brane Inflation, Solitons and Cosmological Solutions: I
• Late time sky as a probe of steps and oscillations in primordial Universe
• Using the filaments in the LCRS to test the LambdaCDM model
• Lepton number violation in Little Higgs model
• Interacting Tsallis and Rényi Holographic Dark Energy with Hybrid Expansion Law
• Constraining the interacting dark energy models from weak gravity conjecture and recent observations
• Cosmological constraints on polytropic gas model
• Numerical solutions to Einstein's equations in a shearing-dust Universe: a code comparison
• Noether Symmetry Analysis of Anisotropic Universe in Modified Gravity
• Signals of dark matter in a supersymmetric two dark matter model
• Probing Dark Energy with Supernovae : Bias from the time evolution of the equation of state
• Viscous universe with cosmological constant
• Parameterizing the Power Spectrum: Beyond the Truncated Taylor Expansion
• Dark Energy: The Observational Challenge
• Prospects for Dark Energy Evolution: a Frequentist Multi-Probe Approach
• New constraint on the cosmological background of relativistic particles
• Imperfect fluid cosmological model in modified gravity
• On the Emergence of Accelerating Cosmic Expansion in f(R) Theories of Gravity
• Latest data constraint of some parameterized dark energy models
• Perturbations for transient acceleration
• The orbit of Beta Pic b as a transiting planet
• Breaking the cosmological background degeneracy by two-fluid perturbations in f(R) gravity
• Small scale clustering of late forming dark matter
• On the consistency of tachyon warm inflation with viscous pressure
• Dark energy, curvature, and cosmic coincidence
• Raytracing simulations of coupled dark energy models
• Testing cosmological models and understanding cosmological parameter determinations with metaparameters
• Noether Symmetries and Anisotropic Universe in Energy-Momentum Squared Gravity
• Barrow Holographic Dark Energy Model with GO Cut-off -- An Alternative Perspective
• Stability of Accelerated Expansion in Nonlinear Electrodynamics
• The Hubble Constant from Type Ia Supernova Calibrated with the Linear and Non-Linear Cepheid Period-Luminosity Relation
• Phase-space of flat Friedmann-Robertson-Walker models with both a scalar field coupled to matter and radiation
• Scalar Field Reconstruction of Power-Law Entropy-Corrected HDE
• Multiple scalar particle decay and perturbation generation
• Mimetic Attractors
• The arbitrariness of potentials in interacting quintessence models
• Lepton flavor violating signals of a little Higgs model at the high energy linear $e^{+}{e}^{-}$ colliders
• Cosmological implications of Rastall-$f(R)$ theory
• Phase Space Analysis and Thermodynamics of Interacting Umami Chaplygin gas in FRW Universe
• Lagrangian theory for cosmic structure formation with vorticity: Newtonian and post-Friedmann approximations
• Distance-redshift from an optical metric that includes absorption
• The Effect of Substructure on Mass Estimates of Galaxies
• Neutrino mass and asymmetric dark matter: study with inert Higgs doublet and high scale validity
• Generalized holographic Ricci dark energy and generalized second law of thermodynamics in Bianchi Type I universe
• The Exoplanet Simple Orbit Fitting Toolbox (ExoSOFT): An Open-Source Tool for Efficient Fitting of Astrometric and Radial Velocity Data
• Improved model-independent constraints on the recombination era and development of a direct projection method
• Charged gravastar model in Rastall theory of gravity
• A Complete Cosmological Scenario in Teleparallel Gravity
• Inflation with F(T) Teleparallel Gravity
• Dilaton dominance in the early Universe dilutes Dark Matter relic abundances
• Stochastic gravitational wave background from cold dark matter halos
• Gravitational waves in the generalized Chaplygin gas model
• Theoretical Limits on Agegraphic Quintessence from Weak Gravity Conjecture
• Observational constraints on unified dark matter including Hubble parameter data
• Power-law entropy-corrected HDE and NADE in Brans-Dicke cosmology
• Ballistic Dark Matter oscillates above $\Lambda$CDM
• Self accelerating solutions in a DGP brane with a scalar field trapped on it: the dynamical systems perspective
• Growth of perturbations in dark energy parametrization scenarios
• Inflation in a modified radiative seesaw model
• A Two-field Dilaton Model of Dark Energy
• f(T) cosmology against the cosmographic method: A new study using mock and observational data
• QCD modified ghost scalar field dark energy models
• Supersymmetric extra U(1) models with a singlino dominated LSP
• Affleck-Dine leptogenesis in the radiative neutrino mass model
• Singlino dominated LSP as CDM candidate in supersymmetric models with an extra U(1)
• Single production of the doubly charged scalar in the littlest Higgs model
• Probing Dark Energy with Supernovae : a concordant or a convergent model?
• Constraints on Dark Matter-Neutrino Interaction from 21-cm Cosmology and Forecasts on SKA1-Low
• The Nature of Obscuration in AGN: I. Insights from Host Galaxies
• Explicit CP violation in a MSSM with an extra $U(1{)}^{\prime }$
• Inflationary Dynamics and Particle Production in a Toroidal Bose-Einstein Condensate
• Possible features of galactic halo with electric field and observational constraints
• Reconstructing Dark Energy Potentials From Parameterized Deceleration Parameters
• A semi-analytical approach to perturbations in mutated hilltop inflation
• Crossing the cosmological constant line in a dilatonic brane-world model with and without curvature corrections
• Characterising the signatures of star-forming galaxies in the extra-galactic $\gamma$-ray background
• Double beta decay versus cosmology: Majorana CP phases and nuclear matrix elements
• Normalization of the Matter Power Spectrum via Higher-Order Angular Correlations of Luminous Red Galaxies
• Future state of the Universe
• Higgs bosons of a supersymmetric $E_6$ model at the Large Hadron Collider
• Reconstruction of Scalar Field Dark Energy Models in Kaluza-Klein Universe
• Dark matter interacts with variable vacuum energy
• Equation of State of Neutron Stars with Junction Conditions in the Starobinsky Model
• Dark Energy and Neutrino CPT Violation
• The power spectrum from the angular distribution of galaxies in the CFHTLS-Wide fields at redshift ~0.7
• Evolution of Anisotropies in Eddington-Born-Infeld Cosmology
• $f(T)$ non-linear massive gravity and the cosmic acceleration
• Interacting entropy-corrected holographic dark energy with apparent horizon as an infrared cutoff
• On FRW Model in Conformal Teleparallel Gravity
• The Angular Power Spectrum of the First-Year WMAP Data Reanalysed
• Optimized supernova constraints on dark energy evolution
• Neutrino Mass Inference from SZ Surveys
• Curvaton Scenario with Affleck-Dine Baryogenesis
• Lensing as a Probe of Early Universe: from CMB to Galaxies
• Modified Gauss-Bonnet Gravity with Radiating Fluids
• Structure formation in dark energy cosmologies described by PADE parameterization
• Cosmological constrains from X-ray AGN clustering and SNIa data
• Kaluza-Klein Cosmology with Varying G and $\Lambda$
• Noether symmetry in a nonlocal f(T) Gravity
• Dark Energy Models With Variable Equation Of State Parameter
• On Weyl cosmology in five dimensions and the cosmological constant
• Accelerating Hilbert-Einstein universe without dynamic dark energy
• On the Gravitational Energy-Momentum Vector in f(T) Theories
• Analytic Solutions and Observational support: A study of $f(R,T)$ gravity with $f(R,T)=R+h(T)$
• Interacting Holographic Dark Energy, the Present Accelerated Expansion and Black Holes
• Statefinder Parameters for Different Dark Energy Models with Variable G Correction in Kaluza-Klein Cosmology
• Bianchi Type-I Universe Models with Nonlinear Viscosity
• Cosmological neutrino mass limit and the dynamics of dark energy
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• Cosmological Solutions with Torsion in a Model of de Sitter Gauge Theory of Gravity
• Do recent observations favor a cosmological event horizon: A thermodynamical prescription?
• Asymptotic Analysis of the Boltzmann Equation for Dark Matter Relics
• Cosmological reconstruction and {\it Om} diagnostic analysis of Einstein-Aether Theory
• Dynamical Models for NGC 6503 using a Markov Chain Monte Carlo Technique
• Speeding Up Cosmological Boltzmann Codes
• Holographic Dark Energy Like in $f(R)$ Gravity
• Holographic dark energy interacting with dark matter in a Closed Universe
• Lepton number asymmetry via inflaton decay in a modified radiative seesaw model
• Cosmological Evolution of Pilgrim Dark Energy
• Five-dimensional metric $f(R)$ gravity and the accelerated universe
• Weinberg's Higgs portal confronting recent LUX and LHC results together with upper limits on B^+ and K^+ decay into invisibles
• Delayed Recombination and Standard Rulers
• Cosmic Acceleration and Brans-Dicke Theory
• Dark world and baryon asymmetry from a common source
• Designer de Sitter Spacetimes
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• The generalized second law for the interacting new agegraphic dark energy in a non-flat FRW universe enclosed by the apparent horizon
• New parameterization for unified dark matter and dark energy
• Logarithmic entropy corrected holographic dark energy with $F(R,T)$ gravity
• Momentum transfer in the dark sector and lensing convergence in upcoming galaxy surveys
• Topology and geometry of the dark matter web: a multistream view
• Scalar field-perfect fluid correspondence and nonlinear perturbation equations
• Static Spherically Symmetric Solution of (R +- μ^4/R) Gravity
• Holographic Dark Energy Characterized by the Total Comoving Horizon and Insights to Cosmological Constant and Coincidence Problem
• Matter Power Spectrum for Convex Quartessence
• FLRW accelerating universe with interactive dark energy
• A new parametrization for dark energy density and future deceleration
• Interacting entropy-corrected holographic Chaplygin gas model
• Tachyon warm inflationary universe model in the weak dissipative regime
• De Sitter Thermodynamics from Diamonds's Temperature
• Chameleon Field Dynamics During Inflation
• Asymmetric Swiss-cheese brane-worlds
• Constraining a double component dark energy model using type Ia supernovae data
• The effects of the small-scale behaviour of dark matter power spectrum on CMB spectral distortion
• Imprints of non-standard Dark Energy and Dark Matter Models on the 21cm Intensity Map Power Spectrum
• The Integrated Sachs-Wolfe Effect in Time Varying Vacuum Model
• Dynamics of Axial Symmetric System in Self-Interacting Brans-Dicke Gravity
• Gauge-ready formulation of cosmological perturbations in scalar-vector-tensor theories
• Analysis of $f(R)$ Theory Corresponding to NADE and NHDE
• A stable flat entropy-corrected FRW universe
• Interacting Viscous Dark Energy in Bianchi Type-I Universe
• Ricci-Gauss-Bonnet holographic dark energy in Chern-Simons modified gravity: A flat FLRW quintessence-dominated universe
• Improving Dark Energy Constraints with High Redshift Type Ia Supernovae from CANDELS and CLASH
• Cosmological constraints on holographic dark energy models under the energy conditions
• Detecting the neutral IGM in filaments with the SKA
• Observational constraints on a cosmological model with Lagrange multipliers
• Correlation function: biasing and fractal properties of the cosmic web
• An FLRW interacting dark energy model of the Universe
• Holographic Dark Energy Model Characterized by the Conformal-age-like Length
• Generalized Self-similar Scalar-Tensor Theories
• Dynamics of interacting scalar field model in the realm of chiral cosmology
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• How accurate is our knowledge of galaxy bias?
• Dark Energy Nature in Logarithmic $f(R,T)$ Cosmology
• A model for Neutrino Masses and Dark Matter with the Discrete Gauge Symmetry
• Searching for blue in the dark
• Constraints on Dark Energy Models Using Late Universe Probes
• Hybrid dark energy
• Dynamic Field Theory and Equations of Motion in Cosmology
• Keck Spectroscopy of Globular Clusters in the Virgo Cluster Dwarf Elliptical VCC 1386
• Observational Constraints on Undulant Cosmologies
• Periodic Cosmological Evolutions of Equation of State for Dark Energy
• A Dark Energy Model in Lyra Manifold
• A New Class of Bianchi Type-I Cosmological Models in Scalar-Tensor Theory of Gravitation and Late Time Acceleration
• Cosmic rays at ultra high energies (Neutrinos!)
• An indirect limit on the amplitude of primordial Gravitational Wave Background from CMB-Galaxy Cross Correlation
• Surveying the dark side
• Constraining the CDM spectrum normalization in flat dark energy cosmologies
• Can Strong Gravitational Lensing Constrain Dark Energy?
• Decoupling Dark Energy from Matter
• Evidence for new physics from clusters ?
• Cosmology from String Theory
• Electromagnetic Leptogenesis
• Cosmological zoo -- accelerating models with dark energy
• Noether symmetry in the Nash theory of gravity
• Whether Lyra's Manifold Itself is a Hidden Source of Dark Energy
• Tracking Quintessence and Cold Dark Matter Candidates
• Cosmic Voids in Evolving Dark Sector Cosmologies: the Low Redshift Universe
• Cosmology With A Dark Refraction Index
• Interacting holographic Ricci dark energy as running vacuum
• Dynamical systems of cosmological models for different possibilities of $G$ and ${\rho }_{\Lambda }$
• Modeling galactic halos with predominantly quintessential matter
• Implications of Halo Inside-out Growth on the X-Ray Properties of Nearby Galaxy Systems within the Preheating Scenario
• Scalar Triplet Flavor Leptogenesis with Dark Matter
• Observational constraints on finite scale factor singularities
• Power-law entropy corrected new holographic scalar field models of dark energy with modified IR-cutoff
• Lorentzian wormhole in the framework of loop quantum cosmology
• ISW-Galaxy Cross Correlation:A probe of Dark Energy clustering and distribution of Dark Matter tracers
• Extra-Dimensions and Dark Matter
• Quantum cosmic models and thermodynamics
• Inflation due to a non-minimal coupling of singlet scalars in the radiative seesaw model
• Twenty-One New Light Curves of OGLE-TR-56b: New System Parameters and Limits on Timing Variations
• Flux Compactifications: Stability and Implications for Cosmology
• Power-law solutions and accelerated expansion in scalar-tensor theories
• Bianchi type-V dark energy model with varying EoS parameter
• Holographic dark energy with time varying $c^2$ parameter
• Exploring Plane Symmetric Solutions in $f(R)$ Gravity
• Stable Large-Scale Perturbations in Interacting Dark-Energy Model
• The Monge-Ampère-Kantorovich approach to reconstruction in cosmology
• $Om$ Diagnostic for Dilaton Dark Energy
• FRW dark energy cosmological model with hybrid expansion law
• Holographic dark energy with time depend gravitational constant in the non-flat Ho$\check{r}$ava-Lifshitz cosmology
• Transient acceleration in $f(T)$ gravity
• Symmetric-Bounce Quantum State of the Universe
• Statefinder diagnostic of logarithmic entropy corrected holographic dark energy with Granda-Oliveros IR cut-off
• Charged gravastar model in $f(T)$ gravity admitting conformal motion
• CMBR Weak Lensing and HI 21-cm Cross-correlation Angular Power Spectrum
• Implications of Rastall Theory on Stellar Solutions admitting Vanishing Complexity: A New Perspective
• ISW-LSS cross-correlation in coupled Dark Energy models with massive neutrinos
• Universe Bounded By Event Horizon: A Non equilibrium Thermodynamic Prescription
• Observational constraints on the braneworld model with brane-bulk energy exchange
• Weyl Anomaly and Initial Singularity Crossing
• Interacting holographic dark energy models: A general approach
• Asymptotic behavior of Cardassian cosmologies with exponential potentials
• A Quintessentially Geometric Model
• On existence of a possible Lorentz invariant modified gravity in Weitzenböck spacetime
• Interacting generalized ghost dark energy in non-flat universe
• Power-Law and Logarithmic Entropy-Corrected Ricci Viscous Dark Energy and Dynamics of Scalar Fields
• Instant nonthermal leptogenesis
• Cosmic Voids in Evolving Dark Sector Cosmologies: the High Redshift Universe
• Bianchi type-VI anisotropic dark energy model with varying EoS parameter
• Nonsingular density profiles of dark matter halos and Strong gravitational lensing
• Recovering Cosmic Microwave Background Polarization Signals with Machine Learning
• Testing the growth rate in homogeneous and inhomogeneous interacting vacuum models
• Observational constraints on the fractal cosmology
• Probing for variation of neutrino mass with current observations
• Sneutrino inflation in Gauss-Bonnet brane-world cosmology, the gravitino problem and leptogenesis
• Holographic Dark Energy Interacting with Two Fluids and Validity of Generalized Second Law of Thermodynamics
• Lepton mass and mixing in a Neutrino Mass Model based on $S_4$ flavor symmetry
• Qualitative description of the universe in the interacting fluids scheme
• Chaotic dynamics in preheating after inflation
• A Modified Generalized Chaplygin Gas as the Unified Dark Matter-Dark Energy Revisited
• Nonbaryonic dark matter and scalar field coupled with a transversal interaction plus decoupled radiation
• (m,n)-type holographic dark energy models
• Effects of structure formation on the expansion rate of the Universe: An estimate from numerical simulations
• Solar System Constraints on a Cosmologically Viable $f(R)$ Theory
• Dark Matter Decaying into a Fermi Sea of Neutrinos
• Holographic dark energy in Barrow cosmology with Granda-Oliveros IR cutoff
• Relaxing the Cosmological Constraints on Unparticle Dark Component
• Non-flat universe and interacting dark energy model
• Cosmological determination to the values of the prefactors in the logarithmic corrected entropy-area relation
• Interacting holographic dark energy in the scalar-Gauss-Bonnet gravity
• Probing galaxy density profiles with future supernova surveys
• On The Temporal Evolution of Particle Production in $f(T)$ Gravity
• Generalized second law of thermodynamics in QCD ghost f(G) gravity
• Dark Energy Cosmology with the Alternative Cosmic Microwave Background Data
• The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity in Bianchi-I spacetime
• Constraints on $\Lambda (t)$-cosmology with power law interacting dark sectors
• Observational Constraints on the Generalized Chaplygin Gas
• Limits from Weak Gravity Conjecture on Dark Energy Models
• Bianchi type-I string cosmological model in the presence of a magnetic field: classical versus loop quantum cosmology approaches
• Interacting new agegraphic Phantom model of dark energy in non-flat universe
• Consequences of dark matter self-annihilation for galaxy formation
• Consistency of nonlinear interacting ghost dark energy with recent observations
• Detecting dark energy in long baseline neutrino oscillations
• A spherical scalar-tensor galaxy model
• Multi-(super)graviton theory on topologically non-trivial backgrounds
• Chaplygin Gas Hořava-Lifshitz Quantum Cosmology
• Observationally constrained accelerating cosmological model with higher power of non-metricity and squared trace
• Dynamical features of $f(T,B)$ cosmology
• Constraining Holographic Dark Energy and Analyzing Cosmological Tensions
• Non-minimally coupled quintessence DE model with a cubic galileon term --A Dynamical System Analysis
• Holographic dilatonic model of dark energy
• CSST Large-scale Structure Analysis Pipeline: II. the CSST Emulator for Slitless Spectroscopy (CESS)
• Alternative High-z Cosmic Tracers and the Dark Energy Equation of State
• A model of dark matter dark energy interaction with some cosmic consequences
• Cosmologies with variable parameters and dynamical cosmon: implications on the cosmic coincidence problem
• Crossing the Phantom Divide in Extended Dvali-Gabadadze-Porrati Gravity
• F(R) cosmology via Noether symmetry and lambda-Chaplygin Gas like model
• Ellipticals at z=0 from Self-Consistent Hydrodynamical Simulations: Clues on Age Effects in their Stellar Populations
• First Axion-Like Particle Results from a Broadband Search for Wave-Like Dark Matter in the 44 to 52 $\mu$eV Range with a Coaxial Dish Antenna
• The CMBR ISW and HI 21-cm Cross-correlation Angular Power Spectrum
• Halting eternal acceleration with an effective negative cosmological constant
• Higher Dimensional Dark Energy Investigation with Variable $\Lambda$ and $G$
• Modeling and Analyzing Stability of Hybrid Stars within $f(Q)$ Gravity
• Real space tomography of the primordial Universe with cluster polarization
• Cosmological dynamics of a non-minimally coupled bulk scalar field in DGP setup
• Cosmological constraints on Agegraphic dark energy in DGP braneworld gravity
• Scale dependence of the primordial spectrum from combining the three-year WMAP, Galaxy Clustering, Supernovae, and Lyman-alpha forests
• Is flat rotation curve a sign of cosmic expansion?
• Long Gamma-Ray Burst prompt emission properties as a cosmological tool
• F_D-Term Hybrid Inflation with Electroweak-Scale Lepton Number Violation
• Dark Energy as Double N-Flation--Observational Predictions
• de Sitter Harmonies: Cosmological Spacetimes as Resonances
• Evolution of superclusters and supercluster cocoons in various cosmologies
• Cosmological Constraint and Analysis on Holographic Dark Energy Model Characterized by the Conformal-age-like Length
• Time Variable Cosmological Constants from the Age of Universe
• Modelling Tachyon Cosmology with Non-Minimal Derivative Coupling to Gravity
• Cosmic acceleration and phantom crossing in $f(T)$-gravity
• Classification of Cosmic Scale Factor via Noether Gauge Symmetries
• Irreversible thermodynamics of dark energy on entropy-corrected apparent horizon
• Leptonic Dark Energy and Baryogenesis
• Reconstructing $f(T)$ modified gravity from ECHDE and ECNADE models
• Fingerprints of Anomalous Primordial Universe on the Abundance of Large Scale Structures
• First-order formalism for the quintom model of dark energy
• A Cosmological Model with Dark Spinor Source
• Uncertainties in the S-Z selected cluster angular power spectrum
• N-body simulations, halo mass functions, and halo density profile in $f(T)$ gravity
• The biasing phenomenon
• Fractal FRW Model within Domain Wall
• Polytropic gas scalar field models of dark energy
• Stability analysis in Modified Non-Local Gravity
• Interacting agegraphic dark energy models in phase space
• Revisit of constraints on dark energy with Hubble parameter measurements including future redshift drift observations
• X-ray Clusters of Galaxies as Cosmological Tools
• Constraint on dark matter central density in the Eddington inspired Born-Infeld (EiBI) gravity with input from Weyl gravity
• Closed inflationary universe with tachyonic field
• Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
• The Logotropic Dark Fluid: Observational and Thermodynamic Constraints
• Dilaton dominance relaxes LHC and cosmological constraints in supersymmetric models
• Interacting holographic tachyon model of dark energy
• On Internal Consistency of Holographic Dark Energy Models
• Astrophysical Observations: Lensing and Eclipsing Einstein's Theories
• Bohmian Quantization of the Big Rip
• Interacting Agegraphic Dark Energy Model in DGP Braneworld Cosmology: Dynamical System Approach
• Cosmological Analysis of Modified Holographic Ricci Dark Energy in Chern-Simons Modified Gravity
• A Comparison of Quintessence and Nonlinear Born-Infeld Scalar Field Using Gold Supernova data
• Towards a possible solution for the coincidence problem: f(G) gravity as background
• Phantom fields: bounce solutions in the early Universe and S-branes
• Thermodynamics in a Modified Gravity Involving Higher-Order Torsion Derivative Terms
• The Effective Fluid approach for Modified Gravity and its applications
• Anisotropy effects on Baryogenesis in $f(R)$-Theories of Gravity
• Evolution of linear perturbations through a bouncing world model: Is the near Harrison-Zel'dovich spectrum possible via a bounce?
• Atmospheric Scintillation Noise in Ground-Based Exoplanet Photometry
• Modified holographic Ricci dark energy coupled to interacting relativistic and non-relativistic dark matter in the nonflat universe
• Evolution of magnetic component in Yang-Mills condensate dark energy models
• Massive Neutrinos in Cosmology
• Matrix Formalism of Excursion Set Theory: A new approach to statistics of dark matter halo counting
• Observational Constraints on Varying Alpha in $\Lambda (\alpha )$CDM Cosmology
• Quantum Yang--Mills Dark Energy
• Energy Constraints and $F(T,T_G)$ Cosmology
• Physical condition for the slowing down of cosmic acceleration
• Power suppression from disparate mass scales in effective scalar field theories of inflation and quintessence
• Generalized Model for $\Lambda$-Dark Energy
• Dark Energy and Modified Scale Covariant Theory of Gravitation
• Perturbation level interacting dark energy model and its consequence on late-time cosmological parameters
• Is the CMB shift parameter connected with the growth of cosmological perturbations?
• Dynamics of Brans-Dicke cosmology with varying mass fermions
• Simultaneous effect of Modified Gravity and Primordial Non-Gaussianity in Large Scale Structure Observations
• Neutralino relic density from ILC measurements in the CPV MSSM
• An extension of the cosmological standard model with a bounded Hubble expansion rate
• Reconstructions of $f(\mathcal{P})$ and $f(\mathcal{Q})$ gravity models from $(m,n)$-type Barrow Holographic Dark Energy: Analysis and Observational Constraints
• Analytical solutions of the geodesic equation in the space-time of a black hole surrounded by perfect fluid in Rastall theory
• Statistical characteristics of observed Ly-$\alpha$ forest and the shape of initial power spectrum
• Weak Interaction Rate Coulomb Corrections in Big Bang Nucleosynthesis
• On the stability of the dark energy based on generalized uncertainty principle
• Perturbation Spectra of Warm Inflation in $f(Q,T)$ Gravity
• Interacting warm dark matter
• Multi-band characterization of the hot Jupiters: WASP-5b, WASP-44b and WASP-46b
• Observational Constraints on Visser's Cosmological Model
• Unifying static analysis of gravitational structures with a scale-dependent scalar field gravity as an alternative to dark matter
• Heavy Higgs Resonances for the Neutralino Relic Density in the Higgs Decoupling Limit of the CP--noninvariant Minimal Supersymmetric Standard Model
• Neutrino Mass Limit from Galaxy Cluster Number Density Evolution
• Ghost dark energy with sign-changeable interaction term
• Tachyonic (phantom) power-law cosmology
• Pair production of charged scalars and lepton flavor violating signals in the littlest Higgs model at $e^{+}{e}^{-}$ colliders
• Selection effects on X-ray and strong-lensing clusters in various cosmologies
• Effect of low anisotropy on cosmological models by using supernova data
• Fischler-Susskind holographic cosmology revisited
• Mixed fluid cosmological model in $f(R,T)$ gravity
• Phantom-Like Behavior of a DGP-Inspired Scalar-Gauss-Bonnet Gravity
• Entropy-corrected new agegraphic dark energy in Horava-Lifshitz cosmology
• Early and Late-time Cosmic Acceleration in Non-minimal Yang-Mills-$f(G)$ Gravity
• The accelerated scaling attractor solution of the interacting agegraphic dark energy in Brans-Dicke theory
• Discord in Concordance Cosmology and Anomalously Massive Early Galaxies
• Inflation and New Agegraphic Dark Energy
• The XMM Cluster Survey: The Halo Occupation Number of BOSS galaxies in X-ray clusters
• Potentialities of Hubble parameter and expansion rate function data to alleviate Hubble tension
• Knot Universes in Bianchi Type I Cosmology
• Exact solution to perturbative conformal cosmology in the recombination era
• Baryon asymmetry from leptogenesis with four zero neutrino Yukawa textures
• Generalized second law of thermodynamics in presence of interacting DBI essence and other dark energies
• Age problem in holographic dark energy
• Rapid onset of the 21-cm signal suggests a preferred mass range for dark matter particle
• Dynamics of Void and its Shape in Redshift Space
• Statistical characteristics of observed Ly-$\alpha$ forest and the shape of linear power spectrum
• Testing feasibility of scalar-tensor gravity by scale dependent mass and coupling to matter
• A way to get rid of cosmological constant and zero point energy problems of quantum fields through metric reversal symmetry
• Bouncing cosmological models in a functional form of F(R) gravity
• Observational constraints and stability in viscous $f(T,\mathcal{T})$ gravity
• Dissecting Galaxies with Quantitative Spectroscopy of the Brightest Stars in the Universe
• The tension of cosmological magnetic fields as a contribution to dark energy
• Cosmological black holes as voids progenitors. I. Simulations
• Testing self-interacting dark matter with galaxy warps
• Resolving FLRW cosmology through effective equations of state in $f(T)$ gravity
• Viscous Dark Energy and Phantom Field in An Anisotropic Universe
• Observational Constraints of Homogeneous Higher Dimensional Cosmology with Modified Chaplygin Gas
• Baryogenesis with Superheavy Squarks
• Extended Bose-Einstein condensate dark matter in viscous Gauss-Bonnet gravity
• Dark energy in thermal equilibrium with the cosmological horizon?
• The extragalactic $\gamma$-ray background: imprints from the physical properties and evolution of star-forming galaxy populations
• Reconstruction of the equation of state for the cyclic universes in homogeneous and isotropic cosmology
• A new model for dark matter fluid sphere
• The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
• First step toward matter power spectrum reconstruction with Stage III weak gravitational lensing surveys
• Gauss-Bonnet braneworld and WMAP three year results
• Noncommutative Universe and Chameleon Field Dynamics
• Cosmic evolution in the background of non-minimal coupling in $f(R,T,R_{\mu \nu }{T}^{\mu \nu })$ Gravity
• Stable $f(Q)$ gravity model through non-trivial connection
• Newman-Penrose formalism and exact vacuum solutions to conformal Weyl gravity
• Fermion Mass and Mixing in a Low-Scale Seesaw Model based on the S4 Flavor Symmetry
• Cosmological perturbation and matter power spectrum in bimetric massive gravity
• The Gravitational Deflection of Light in F(R)-gravity
• Dynamical systems analysis of an interacting scalar field model in an anisotropic universe
• Coupled Quintessence scalar field model in light of observational datasets
• Thermodynamics of dynamical wormholes
• Phantom energy from graded algebras
• Non-adiabatic perturbations in Ricci dark energy model
• Lyman-alpha forest-CMB cross-correlation and the search for the ionized baryons at high redshift
• No-Bang Quantum State of the Cosmos
• Coupled scalar field cosmology with effects of curvature
• Dynamics of Mixed Dark Energy Domination in Teleparallel Gravity and Phase-Space Analysis
• Observational Hubble parameter data constraints on the interactive model of $f(T)$ gravity with particle creation
• CoRoT LRa02_E2_0121: Neptune-size planet candidate turns into a hierarchical triple system with a giant primary
• Cosmological solutions in spatially curved universes with adiabatic particle production
• The interaction of extended Bose-Einstein condensate dark matter with viscous $f(T,B)$ gravity
• Quantum induced w = -1 crossing of the quintessence and phantom models
• Nonsingular Chaplygin gas cosmologies in universes connected by wormhole
• Stability of neutron stars in Horndeski theories with Gauss-Bonnet couplings
• Low energy conversion electron detection in superfluid He3 at ultra-low temperature
• Reconstructing quintom from WMAP 5-year observations: Generalized ghost condensate
• $Z_L$ associated pair production of charged Higgs bosons in the littlest Higgs model at $e^{+}{e}^{-}$ colliders
• Probing Ricci dark energy model with perturbations by using WMAP seven-year cosmic microwave background measurements, BAO and Type Ia supernovae
• Ricci curvature non-minimal derivative coupling cosmology with field re-scaling
• Non-local scalar fields inflationary mechanism in light of Planck $2013$
• Hidden from view: Coupled Dark Sector Physics and Small Scales
• Refining the predictions of supersymmetric CP-violating models: A top-down approach
• Detectability of Cosmic Topology in Generalized Chaplygin Gas Models
• Voids and overdensities of coupled Dark Energy
• Spacetime averaging of exotic singularity universes
• A symmetry for vanishing cosmological constant
• Neutrino masses and $\mu$ terms in a supersymmetric extra U(1) model
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• Fitting of supernovae without dark energy
• Self-shielding effect of a single phase liquid xenon detector for direct dark matter search
• Strong and weak gravitational field in $R+{\mu }^4/R$ gravity
• Analysis cosmological tachyon and fermion model and observation data constraints
• Surface Tension: Accelerated Expansion, Coincidence Problem & Hubble Tension
• Constraining Parameters for the Accelerating Universe in $f(R,{\mathcal{L}}_m)$ Gravity
• Dark energy from topology change induced by microscopic Gauss-Bonnet wormholes
• Modified gravity in a viscous and non-isotropic background
• From the Spectrum to Inflation: A Second Order Inverse Formula for the General Slow-Roll Spectrum
• "Expansion" around the vacuum: how far can we go from Lambda?
• Quantized cosmological constant in 1+1 dimensional quantum gravity with coupled scalar matter
• Neutralino annihilation beyond leading order
• Formation of First Stars Triggered by Collisions and Shockwaves: Prospect for High Star Formation Efficiency and High Ionizing Photon Escape Fraction
• Coincidence Problem in f(T) Gravity Models
• A numerical approach to model independently reconstruct $f(R)$ functions through cosmographic data
• Towards an Observational Appraisal of String Cosmology
• Constraining Parameters of Generalized Cosmic Chaplygin Gas in Loop Quantum Cosmology
• Holographic Dark Energy with Time Varying n^2 Parameter in Non-Flat Universe
• Observational Consequences of Quantum Cosmology
• Dark energy in hybrid inflation
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• Rare Weak Decays and Direct Lepton Number Violating Signals in a Minimal R-Parity Violating Model of Neutrino Mass
• Anisotropic Dark Energy and the Generalized Second Law of Thermodynamics
• Distances to Galaxies from the Brightest Stars in the Universe
• Dynamics of k-essence in loop quantum cosmology
• Z-bursts from the Virgo cluster
• Is the physics within the Solar system really understood?
• Correlated Mixture Between Adiabatic and Isocurvature Fluctuations and Recent CMB Observations
• Re-examining the role of curvature in the slowing down acceleration scenario
• Galactic cluster winds in presence of a dark energy
• Observational Constraints of Modified Chaplygin Gas in RS II Brane
• Cosmological bounds on masses of neutrinos and other thermal relics
• The Quest for the Inflationary Spectral Runnings in the Presence of Systematic Errors
• Structure formation in clustering DBI dark energy model with constant sound speed
• The quintessence scalar field in the relativistic theory of gravity
• Phase space analysis of some interacting Chaplygin gas models
• New Inflation vs. Chaotic Inflation, Higher Degree Potentials and the Reconstruction Program in light of WMAP3
• Late cosmic acceleration in a vector--Gauss-Bonnet gravity model
• Randers geometry as MOND/dark matter
• Understanding Galaxy Formation and Evolution
• Interacting Kasner-type cosmologies
• Study of Majorana Fermionic Dark Matter
• Dynamics of entropy perturbations in assisted dark energy with mixed kinetic terms
• Summary of ICHEP 2004
• Phantom Divide Crossing with General Non-minimal Kinetic Coupling
• Observational constraints on the unified dark matter and dark energy model based on the quark bag model
• Indirect Detection of Kaluza-Klein Dark Matter from Latticized Universal Dimensions
• Can tides explain the low dark matter density in Fornax?
• Inflation in minimal left-right symmetric model with spontaneous D-parity breaking
• Reconstructing the parameter space of non-analytical cosmological fixed points
• The effect of curvature in thawing models
• Lepton mass and mixing in a simple extension of the Standard Model based on T7 flavor symmetry
• Troubles for observing the inflaton potential
• Investigation of Bouncing Universe and Phantom Crossing in Modified Gravity Coupled with Weyl Tensor and its Reconstruction
• Galaxy clusters in presence of dark energy: a kinetic approach
• $C^{\infty }$ perturbations of FRW models with a cosmological constant
• Dynamics of Potentials in Bianchi Type Scalar-Tensor Cosmology
• An Interacting Scenario for Dark Energy in Bianchi Type-I Universe
• Testing for Features in the Primordial Power Spectrum
• Non-minimal derivative coupling in Palatini cosmology: acceleration in chaotic inflation potential
• Understanding selection effects in observed samples of cataclysmic variables
• New simple and accurate quintessence approximations
• Isochronous Cosmologies
• Effects of particle creation rate in two-fluid interacting cosmologies
• Superluminal apparent motions in distant radio sources
• Future cosmological evolution in $f(R)$ gravity using two equations of state parameters
• Large-scale structure and the Cardassian fluid
• The growth of DM and DE perturbations in DBI non-canonical scalar field scenario
• On the Determination of Neutrino Masses and Dark Energy Evolution from the Cross Correlation of CMB and LSS
• Inflation after WMAP3
• Statistically significant length scale of filaments as a robust measure of galaxy distribution
• Neutrino mass and lepton number violation in the Little Higgs model
• Statefinder analysis of the superfluid Chaplygin gas model
• New holographic Chaplygin gas model of dark energy
• Cosmic Acceleration and Geodesic Deviation in Chameleon Scalar Field Model
• Scalar-Torsion Mode in a Cosmological Model of the Poincaré Gauge Theory of Gravity
• Deciphering the properties of the central engine in GRB collapsars
• Complementarity of Future Dark Energy Probes
• The Bianchi type-V Dark Energy Cosmology in Self Interacting Brans Dicke Theory of Gravity
• Interacting Three Fluid System and Thermodynamics of the Universe Bounded by the Event Horizon
• Interacting dark energy model in the brane scenario: A Dynamical System Analysis
• Dynamical Casimir Effect with Semi-Transparent Mirrors, and Cosmology
• Equilibrium sets in quintom cosmologies: the past asymptotic dynamics
• Structure formation and CMBR anisotropy spectrum in the inflessence model
• Crossing of the Cosmological Constant Boundary - an Equation of State Description
• Low Mass Pseudoscalar Dark Matter in an Extended B - L Model
• Growth of cosmic perturbations in the modified $f(R,T)$ gravity
• de Sitter field equations from quadratic curvature gravity: A group theoretical approach
• Accretion of Holographic Dark Energy : Dependency only upon Horizon Radius of Expanding Universe
• Modeling dark energy through an Ising fluid with network interactions
• Mapping the Cosmological Confidence Ball Surface
• Dark matter mass from relic abundance, an extra $U(1)$ gauge boson, and active-sterile neutrino mixing
• Can the coincidence problem be solved by a cosmological model of coupled dark energy and dark matter?
• Evolution of Dark Energy Perturbations for Slotheon Field and Power Spectrum
• Environmental effects on halo abundance and weak lensing peak statistics toward large underdense regions
• Electromagnetic perturbations of a de Sitter black hole in massive gravity
• A very extended reionization epoch ?
• Vacuum Energy from an Extra Dimension with UV/IR Connection
• Testing the Consistence of Gamma Ray Burst Data-set and Supernovae Union2
• False Vacuum in the Supersymmetric Mass Varying Neutrinos Model
• Modelling Cosmic Acceleration in Modified Yang - Mills Theory
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia, BAO, CMB, H(z) and X-ray gas mass fraction
• Some Specific Wormhole Solutions in Extended $f(R,G,T)$ Gravity
• The Expansion of the Universe and the Cosmological Constant Problem
• Interacting Viscous Dark Energy in Bianchi Type-III Universe
• Observational constraints on tachyonic chameleon dark energy model
• Non-Gaussianity in the warm k-inflation
• Holographic inflation and holographic dark energy from entropy of the anti-de Sitter black hole
• Variable $G$ Correction for Dark Energy Model in Higher Dimensional Cosmology
• A comprehensive analysis of the compact phase space for Hu-Sawicki $f(R)$ dark energy models including spatial curvature
• Dynamical evolution of quintessence cosmology in a physical phase space
• Bulk scalar field in brane-worlds with induced gravity inspired by the $\mathcal{L}(R)$ term
• Mass decomposition of SLACS lens galaxies in Weyl conformal gravity
• The effect of supersymmetry breaking in the Mass Varying Neutrinos
• The Schr$\ddot{o}$dinger-Poisson equations as the large-N limit of the Newtonian N-body system: applications to the large scale dark matter dynamics
• Non-Linearly Interacting Ghost Dark Energy in Brans-Dicke Cosmology
• Cosmological Parameters and Cosmic Topology
• The reheating constraints to natural inflation in Horndeski gravity
• Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model
• Loitering universe models in light of the CMB
• The Co-Evolution of Galaxies and Black Holes: Current Status and Future Prospects
• Abell 370: A Cluster with a Pronounced Triaxial Morphology
• Cosmological future singularities in massive gravity and massive bigravity
• A Scaling Relation in Inhomogeneous Cosmology with k-essence scalar fields
• Dynamics of holographic dark energy with apparent-horizon cutoff and non-minimal derivative coupling gravity in non-flat FLRW universe
• Statefinders and observational measurement of superenergy
• Dark matter annihilation at cosmological redshifts: possible relic signal from annihilation of weakly interacting massive particles
• The torsion cosmology in Kaluza-Klein theory
• Squeezing Full-Shape Dynamical Dark Energy Constraints with Galaxy Alignments
• Non-Minimal Cosmological Model in Modified Yang--Mills Theory
• Simple quantum cosmology: Vacuum energy and initial state
• A Modified FRW Metric to Explain the Cosmological Constant
• HD 42659: The only known roAp star in a spectroscopic binary observed with B photometry, TESS and SALT
• A simple Hubble-like law in lieu of dark energy
• Measuring the flatness of focal plane for very large mosaic CCD camera
• Direct Dark Matter Searches with CDMS and XENON
• Thick DGP braneworlds
• Thermodynamics of the most generalized form of Holographic Dark Energy and some particular cases with Corrected Entropies
• Observational constraints on a Yang-Mills condensate dark energy model
• Power Law and Logarithmic Ricci Dark Energy Models in Horava-Lifshitz Cosmology
• Phase structure of the $O(2)$ ghost model with higher-order gradient term
• A Measurement of The Faint Source Correlation Function in the GOODS and UDF Survey
• Triangular Ring Resonator: Direct measurement of the parity-odd parameters of the photon sector of SME
• Bounding f(R,T) gravity by particle creation
• On the Possibility of Observing the Shapiro Effect for Pulsars in Globular Clusters
• New parameterizations of generalized Chaplygin gas model constrained at background and perturbation levels
• Gauged Supergravities and the Physics of Extra Dimensions
• Hybrid Inflation, Dark Energy And Dark Matter
• Generalized Ghost Pilgrim Dark Energy Fractal Cosmology with Observational Constraint
• Viscous interacting and stability on dark matter Bose-Einstein condensation with modified Chaplygin gas
• Self-interacting Dark Matter with Scalar Dilepton Mediator
• Cross-Correlation Detection of Point Sources in WMAP First Year Data
• Unification of Gravitation, Gauge Field and Dark Energy
• Reconstructions of Einstein-Aether Gravity from Barrow Agegraphic and New Barrow Agegraphic Dark Energy models: Examinations and Observational Limits
• Confronting Dirac Fermionic Dark Matter with Recent Data
• D-bound and Bekenstein bound for McVittie solution surrounded by dark energy cosmological fields
• Inflation is the generic feature of phantom field-not the big-rip
• Effective field theory of coupled dark energy and dark matter
• Forecasting 21-cm power spectrum sensitivity to dark Matter-baryon scattering
• Modified gravity with disappearing cosmological constant
• Cosmological Fluctuations on the Light Cone
• Agegraphic dark energy with the sign-changeable interaction in non-flat universe
• Exact solution to perturbative conformal cosmology from recombination until the current era
• Stochastic contribution to the growth factor in the LCDM model
• Isochronous Spacetimes
• Peaks in the cosmological density field: parameter constraints from 2dF Galaxy Redshift Survey data
• Models of radial velocities and transit light curves
• Study of thermal stability for different dark energy models
• Analytical considerations about the cosmological constant and dark energy
• Density fluctuations on mm and Mpc scales
• $f(R)$ Gravity and Crossing the Phantom Divide Barrier
• Monte Carlo Comparisons to a Cryogenic Dark Matter Search Detector with low Transition-Edge-Sensor Transition Temperature
• Spinor quintom cosmology with intrinsic spin
• Modified cosmology through generalized mass-to-horizon entropy: observational constraints from DESI DR2 BAO data
• Neutrino mass constraint from CMB and its degeneracy with other cosmological parameters
• Dynamical Oscillations in Dark Energy: Joint Constraints on the $w_{sin}$CDM Model from DESI, OHD, and Supernova Samples
• Constraints on the Neutrino Mass from SZ Surveys
• Phase Space Analysis for Anisotropic Universe with Nonlinear Bulk Viscosity
• Imprints of dark matter-massive neutrino interaction in upcoming post-reionization and galaxy surveys
• Supernovae observations and cosmic topology
• A class of regular bouncing cosmologies
• Constraints on Holographic cosmologies from strong lensing systems
• Probing Composite Gravity in Colliders
• Optical dispersion of composite particles consisting of millicharged constituents
• Phenomenology of Absolute Neutrino Masses
• Instability Analysis of Cylindrical Stellar Object in Brans-Dicke Gravity
• Orbital precession and other properties of two-body motion in the presence of dark energy
• A unification of RDE model and XCDM model
• Lepton flavor mixing in the Wolfenstein scheme
• Hubble Tension and Dark Energy in Teleparallel Gauss-Bonnet Gravity: New Constraints from DESI BAO, Pantheon${}^{+}$ and Hubble Data
• The influence of quintessence on the motion of a binary system in cosmology
• A unified model of inflation and dark energy based on the holographic spacetime foam
• Cosmological perturbations for ultra-light axion-like particles in a state of Bose-Einstein condensate
• Unification of Dark Matter and Dark Energy in a Modified Entropic Force Model
• A Shifted View of Fundamental Physics
• Complex supergravity quintessence models confronted with Sn Ia data
• Cosmological constraints from galaxy clustering
• Coupling q-deformed dark energy to dark matter
• Viscous fluid dynamics with decaying vacuum energy density
• Is it possible to observationally distinguish adiabatic Quartessence from LambdaCDM?
• Constraint on $B-L$ cosmic string from leptogenesis with degenerate neutrinos
• A novel model of non-singular oscillating cosmology on flat Randall-Sundrum II braneworld
• A study of multiscale density fluctuation measurements
• Quantifying the sensitivity of Big Bang Nucleosynthesis to isospin breaking with input from lattice QCD
• Method of determining cosmological parameter ranges with samples of candles with an intrinsic distribution
• Constraints on the Sum of Neutrino Masses from Cosmology and their impact on world neutrino data
• A Holographic Energy Model
• Asymptotic Cosmological Behavior of Scalar-Torsion Mode in Poincare Gauge Theory
• Growth of matter perturbations for realistic $F(R)$ models
• G-corrected holographic dark energy model
• Unified first law for traversable wormholes in non-minimal coupling of curvature and matter
• Lensing convergence and anisotropic dark energy in galaxy redshift surveys
• Two body problem in presence of cosmological constant
• Cosmic microwave background limits on spatially homogeneous cosmological models with dark energy
• The Fourth Gravity Test and Quintessence Matter Field
• Natural Coordinate System in Curved Space-time
• Decorrelating the errors of the galaxy correlation function with compact transformation matrices
• A model of inflation independent of the initial conditions, with bounded number of e-folds and n_s larger orsmaller than one
• Inflation constraints for classes of f(R) models
• The ergodicity bias in the observed galaxy distribution
• $f(T)$ gravity from holographic Ricci dark energy model with new boundary conditions
• Domain Wall and Holographic Dark Energy in $f(Q)$ Theory of Gravity
• Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors
• Dark Matter Constituents
• Observational constraints on models of the Universe with time variable Gravitational and Cosmological constants along MOG
• Cosmological constraints from Gauss-Bonnet braneworld with large-field potentials
• Observational Restrictions and Slow-Roll D-brane Inflation in the Special $F(\varphi ,T)$ Gravity
• Can MONDian vector theories explain the cosmic speed up ?
• Is cosmology just a plausibility argument?
• Power-law solutions for TeVeS
• What is there in the black box of dark energy: variable cosmological parameters or multiple (interacting) components?
• Derivation of the cutoff length from the quantum quadratic enhancement of a mass in vacuum energy constant Lambda
• Leptogenesis in a seesaw model with Fritzsch type lepton mass matrices
• Cosmology in holographic non-minimal derivative coupling theory: constraints from inflation and variation of gravitational constant
• Scalar field quasinormal frequencies of Reissner-Nordström black hole surrounded by quintessence by using he continued fraction method
• Stability of curvature perturbation with new covariant form for energy-momentum transfer in dark sector
• On the cosmological viability of the Hu-Sawicki type modified induced gravity
• The Cosmic Microwave Background anisotropies: open problems
• Cosmological constraints on parameters of one-brane models with extra dimension
• Classical and quantum cosmology in $f(T)$-gravity theory: A Noether symmetry approach
• The architecture of the GJ876 planetary system. Masses and orbital coplanarity for planets b and c
• Stability of HDE model with sign-changeable interaction in Brans-Dicke theory
• Thermodynamics and holography of tachyon cosmology
• Star-forming galaxies in the cosmic web in the last 11 Gyr
• Dark energy from conformal symmetry breaking
• The Stability Analysis of Brane Induced Gravity with Quintessence Field on the Brane with a Gaussian Potential
• New Constraints on Dark Energy
• Geometric sigma model of the Universe
• Noether symmetry approach in non-minimal derivative coupling gravity
• Effects of Smoothing Functions in Cosmological Counts-in-Cells Analysis
• Observational constraints on thawing quintessence scalar field model
• Dark matter: A phenomenological existence proof
• Leptogenesis implications in models with Abelian family symmetry and one extra real Higgs singlet
• A non-singular closed bouncing universe without violation of null energy condition
• Modified cosmology through generalized mass-to-horizon entropy: implications for structure growth and primordial gravitational waves
• Higher order mimetic gravity after GW170817
• Weakly Inhomogeneous models for the Low-Redshift Universe
• Exact Cosmological Models with the Yang - Mills Fields on Lyra Manifold
• Pseudo-Scalar Field as a Possible Candidate for Phantom Field
• Exact and Perturbed Friedmann-Lemaitre Cosmologies
• Closed inflationary universe in Patch Cosmology
• Macromodel-free flux-ratio prediction in quadruply imaged quasars with local constraints from lensed arcs
• Chameleon Gravity as an Alternative to Dark Matter
• Reconstructing cosmic evolution with a density parametrization
• Imprint of galactic rotation curves and metric fluctuations on the recombination era anisotropy
• Supersymmetric Lepton Flavor Violation and Leptogenesis
• Three Form Inflation
• Ghosts in the self-accelerating DGP branch with Gauss-Bonnet effect
• Weighing Neutrinos with Large-Scale Structure
• Weak Gravity Conjecture and Holographic Dark Energy Model with Interaction and Spatial Curvature
• Spherical "Top-Hat" Collapse in a Modified Chaplygin Gas Dominated Universe
• The general expression for $f(T)$ in a charged cylindrical spacetime with diverse dimensions
• Quantum hoop conjecture and a natural cutoff for vacuum energy of a scalar field
• Constraining LTB models with JLA supernovae and BAO
• Role of Spatial Curvature in a Dark Energy Interacting Model
• Cosmological volume acceleration in dust epoch: using scaling solutions and variable cosmological term $\Lambda (t)$ within an anisotropic cosmological model
• Inconsistences in Interacting Agegraphic Dark Energy Models
• A dark radiation era prior to the inflationary phase
• Reconstructing f(R) model from Holographic DE: Using the observational evidence
• Evolution of Cluster Alignments as Evidence of Large-scale Structure Formation in the Universe
• Toward accurate measurement of property-dependent galaxy clustering I. Comparison of the Vmax method and the "shuffled" method
• Comparing Production Cross Sections for QCD Matter, Higgs Boson, Neutrino with Dark Energy in Accelerating Universe
• Angular Power Spectrum in Modular Invariant Inflation Model
• (P)reheating Effects of the Kähler Moduli Inflation I Model
• Teleparallel Poincaré Cosmology and $\Lambda$CDM Model
• Static, Cylindrically Symmetric Spacetimes in the Coincident f(Q) Gravity
• Revisiting Agegraphic Dark Energy in Brans-Dicke Cosmology
• On Nash theory of gravity with matter contents
• The Effects of Spatial Curvature on Cosmic Evolution
• Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis
• Cosmological implications of electromagnetically interacting dark matter: milli-charged particles and atoms with singly and doubly charged dark matter
• Optimal-Dimensionality Sampling on the Sphere: Improvements and Variations
• Gravity of Cosmological Perturbations in the CMB
• An analytic approach to the late ISW effect in a Lambda dominated universe
• Falsifying Tree Level String Motivated Bouncing Cosmologies
• Holographic Ricci DE as running vacuum with nonlinear interactions
• Accelerating Kaluza-Klein Universe in Modified Theory of Gravitation
• Gravity and induced matter on Nearly Kahler Manifolds
• How to Measure the Cosmic Curvature
• Isochronous solutions of Einstein's equations and their Newtonian limit
• Late time attractors of some varying Chaplygin gas cosmological models
• Probability of the Initial Conditions for Inflation and Slow Contraction
• Results from Hubble parameter data: oscillating dark energy?
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• Cosmological dynamics of holographic dark energy with non-minimally coupled scalar field
• Cosmology with 21cm intensity mapping
• Spherical Gravitational Collapse of Annihilating Dark Matter and the Minimum Mass of CDM Black Holes
• Optimal Extraction of Cosmological Information from Supernova Data in the Presence of Calibration Uncertainties
• Cosmological Constraints on the Undulant Universe
• Evolution of the horizons for dark energy universe
• Coincidence Problem and Holographic $f(R)$ Gravity in Spatially flat and Curved Universes
• TIC 172900988: A Transiting Circumbinary Planet Detected in One Sector of TESS Data
• On observational signatures of multi-fractional theory
• Spinor-Unit Field Representation of Electromagnetism Applied to a Model Inflationary Cosmology
• K-Inflation with a Dark Energy Coupling
• Unified Model for Inflation and Dark Matter
• Agegraphic dark energy from entropy of the anti-de Sitter black hole
• Precision Cosmology and the Landscape
• Probing Leptophobic Dark Sectors via Gravitational Wave Signatures
• Recent advances in neutrinoless double beta decay search
• Recent Results of non-accelarator-based neutrino experiments
• Getting Information on |U_{e3}|^2 from Neutrino-less Double Beta Decay
• r-Process Enhanced Halo Stars
• Generalized Second Law of Thermodynamics on the Event Horizon for Interacting Dark Energy
• 21-cm power spectrum and ionization bias as a probe of long-mode modulated non Gaussian sky
• Cosmic Microwave Background anisotropies: the power spectrum and beyond
• Semi-holographic model revisited
• Acceleration of the universe in matter dominant era by conformal symmetry breaking
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• Oscillating universe in massive bigravity
• Neutrino cosmology - an update
• Primordial non-Gaussianity systematics from redshift mismatch with SPHEREx
• The effects of a non-zero cosmological constant on the Veltmann models
• Conformal structure of singularities in some varying fundamental constants bimetric cosmologies
• Accelerated expansion of the universe purely driven by scalar field fluctuations
• Nonlinear Spinors as the Candidate of Dark Matter
• Dark Energy Density and IS (Israel-Stewart) Bulk Viscosity Model
• Is cosmic expansion of the universe accelerating?
• $\Lambda$CDM, $\Lambda$DGP and extended phantom-like cosmologies
• The total mass of the early-type galaxy NGC 4649 (M60)
• Possible consistent extra time dimensions in the early universe
• On Gauge Choice of Spherically Symmetric 3-Branes
• Singularities and Soft-Big Bang in a viscous $\Lambda$CDM model
• Stable massless scalar polarization of f(R) gravity
• Comparative Study of $f(T)$ Gravity Models with Observational Constraints from \textit{OHD} and \textit{Pantheon+ datasets}
• Constraints on UED KK-neutrino dark matter from magnetic dipole moments
• Observational Constraints and Cosmological Dynamics of Interacting Fractional Holographic Dark Energy in Light of DESI DR2
• The quintessence field as a perfect cosmic fluid of constant pressure
• Dynamical friction shear and rotation in Chaplygin cosmology
• Inflationary Hubble Parameter from the Gravitational Wave Spectrum in the General Slow-roll Approximation
• On the origin of mid-infrared colors in $\gamma$-ray blazars
• Unified Model for Inflation and the Dark Side of the Universe
• Parametrization of Born-Infeld Type Phantom Dark Energy Model
• Self-restriction of Gravitational Field and its Role in the Universe
• Quintessence reconstruction of interacting HDE in a non-flat universe
• Generalized Eddington--Finkelstein Coordinates and Exact Vaidya-Type Solutions in Weyl Conformal Gravity
• Casimir effect and Stefan-Boltzmann law at finite temperature in a Friedmann-Robertson-Walker universe
• Energy conditions and gravitational baryogenesis in $f(R,\mathcal{R})$ gravity
• Probing Neutrino low energy and mass scales
• Cosmological models with Big rip and Pseudo rip Scenarios in extended theory of gravity
• Phase space analysis of Rényi Holographic dark energy model
• Bouncing Cosmologies in modified gravity with space time torsion
• Power-law and Logarithmic Entropy Corrected Holographic Dark Energy Models in Brans-Dicke Cosmology with Granda-Oliveros Cut-Off
• Cosmic Expansion via Axion-Induced Quintessence
• Agegraphic Model based on the Generalized Uncertainty Principle
• Generalized Noether Theorem for Gauss-Bonnet Cosmology
• Interacting dark matter and q-deformed dark energy non-minimally coupled to gravity
• Effective $\Lambda$CDM model emerging from $f(Q,T)$ under a special EOS limit in symmetric cosmology with Bayesian and ANN observational constraints
• Non-Adiabatic Perturbations from Single-Field Inflation
• Constraints on Energy Conditions in $f(R,L_m)$ Gravity
• The Distortion of the Cosmic Microwave Background by the Milky Way
• Alternative Approaches to Dark Matter Puzzle
• Exploring the Viability of $f(Q,T)$ Gravity: Constraining Parameters with Cosmological Observations
• Geometrothermodynamics of a gravitating system with axially symmetric metric
• Diagnosing Systematic Effects Using the Inferred Initial Power Spectrum
• Manifestations of String Theory in Astrophysical Data and at the LHC
• Using the large scale quasar clustering to constrain flat quintessential universes
• Correspondence between particle creation and dark components interaction in the context of $f(\mathcal{G})$ gravity