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

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