Cosmological Constraints from the SDSS Luminous Red Galaxies

Abstract

We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the Sloan Digital Sky Survey (SDSS) and use this measurement to sharpen constraints on cosmological parameters from the Wilkinson Microwave Anisotropy Probe (WMAP). We employ a matrix-based power spectrum estimation method using Pseudo-Karhunen-Loeve eigenmodes, producing uncorrelated minimum-variance measurements in 20 k-bands of both the clustering power and its anisotropy due to redshift-space distortions, with narrow and well-behaved window functions in the range 0.01h/Mpc < k < 0.2h/Mpc. Results from the LRG and main galaxy samples are consistent, with the former providing higher signal-to-noise. Our results are robust to omitting angular and radial density fluctuations and are consistent between different parts of the sky. They provide a striking confirmation of the predicted large-scale LCDM power spectrum. Combining only SDSS LRG and WMAP data places robust constraints on many cosmological parameters that complement prior analyses of multiple data sets. The LRGs provide independent cross-checks on Om and the baryon fraction in good agreement with WMAP. Within the context of flat LCDM models, our LRG measurements complement WMAP by sharpening the constraints on the matter density, the neutrino density and the tensor amplitude by about a factor of two, giving Omega_m=0.24+-0.02 (1 sigma), sum m_nu < 0.9 eV (95%) and r<0.3 (95%). Baryon oscillations are clearly detected and provide a robust measurement of the comoving distance to the median survey redshift z=0.35 independent of curvature and dark energy properties. Within the LCDM framework, our power spectrum measurement improves the evidence for spatial flatness, sharpening the curvature constraint Omega_tot=1.05+-0.05 from WMAP alone to Omega_tot=1.003+-0.010. Assuming Omega_tot=1, the equation of state parameter is constrained to w=-0.94+-0.09, indicating the potential for more ambitious future LRG measurements to provide precision tests of the nature of dark energy. All these constraints are essentially independent of scales k>0.1h/Mpc and associated nonlinear complications, yet agree well with more aggressive published analyses where nonlinear modeling is crucial.

Matches accepted PRD version. SDSS data, likelihood code, Markov chains and ppt figures available at http://space.mit.edu/home/tegmark/sdss.html 36 journal pages, 25 figs. CosmoMC plugin at http://cosmologist.info/cosmomc/

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• Inflation in Entropic Cosmology: Primordial Perturbations and non-Gaussianities
• On Minimally-Parametric Primordial Power Spectrum Reconstruction and the Evidence for a Red Tilt
• Probing the cosmographic parameters to distinguish between dark energy and modified gravity models
• Tests of Gravity from Imaging and Spectroscopic Surveys
• Imprints of Dark Energy on Cosmic Structure Formation I) Realistic Quintessence Models and the Non-Linear Matter Power Spectrum
• Cosmic Microwave Background Observables of Small Field Models of Inflation
• Coupled quintessence with a $\Lambda$CDM background: removing the ${\sigma }_8$ tension
• Fermion Masses and Flavor Mixings in a Model with $S_4$ Flavor Symmetry
• Constraining the MSSM with universal gaugino masses and implication for searches at the LHC
• Tension of the $E_G$ statistic and RSD data with Planck/$\Lambda$CDM and implications for weakening gravity
• Updated constraints on $f(\mathcal{R})$ gravity from cosmography
• The past and future dynamics of quintom dark energy models
• Dark Energy Survey Year 3 Results: Optimizing the Lens Sample in Combined Galaxy Clustering and Galaxy-Galaxy Lensing Analysis
• Systematic Effects on Determination of the Growth Factor from Redshift-space Distortions
• Constraining cosmological parameters by Gamma Ray Burst X - ray afterglow lightcurves
• SPACE: the SPectroscopic All-sky Cosmic Explorer
• Falsifying Paradigms for Cosmic Acceleration
• Positivity in the sky
• Pilgrim Dark Energy
• Growth Index of DGP Model and Current Growth Rate Data
• Axion isocurvature fluctuations with extremely blue spectrum
• Upper limit for gamma-ray emission above 140 GeV from the dwarf spheroidal galaxy Draco
• Search for Production of Invisible Final States in Single-Photon Decays of Upsilon(1S)
• The Search for a Primordial Magnetic Field
• The VLT LBG Redshift Survey - III. The clustering and dynamics of Lyman-break galaxies at z ~ 3
• Nonlinear growth in modified gravity theories of dark energy
• An improved cosmological bound on the thermal axion mass
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space
• Prospects of inflation in delicate D-brane cosmology
• Thinking Outside the Box: Effects of Modes Larger than the Survey on Matter Power Spectrum Covariance
• Analytical Approach to Subhaloes Population in Dark Matter Haloes
• Constraints on Neutrino Masses from Weak Lensing
• Spherical Collapse in f(R) Gravity
• Estimating the impact of recombination uncertainties on the cosmological parameter constraints from cosmic microwave background experiments
• Running vacuum in the Universe: phenomenological status in light of the latest observations, and its impact on the ${\sigma }_8$ and $H_0$ tensions
• The Millennium Galaxy Catalogue: The local supermassive black hole mass function in early- and late-type galaxies
• Large Scale Structures in Kinetic Gravity Braiding Model That Can Be Unbraided
• Ups and Downs in Dark Energy: phase transition in dark sector as a proposal to lessen cosmological tensions
• Dark Energy Survey Year 3 Results: Measuring the Survey Transfer Function with Balrog
• Present bounds on the relativistic energy density in the Universe from cosmological observables
• Axion constraints in non-standard thermal histories
• Atmospheric Retrieval of Exoplanets
• Axion Inflation and Gravity Waves in String Theory
• A giant ring-like structure at 0.78<z<0.86 displayed by GRBs
• The PAU Survey: Early demonstration of photometric redshift performance in the COSMOS field
• Bulk viscous matter and recent acceleration of the Universe
• Tidal alignments as a contaminant of redshift space distortions
• A 2% Distance to z = 0.35 by Reconstructing Baryon Acoustic Oscillations - III : Cosmological Measurements and Interpretation
• Modelling non-linear redshift-space distortions in the galaxy clustering pattern: systematic errors on the growth rate parameter
• CMB Lensing Constraints on Neutrinos and Dark Energy
• Looking for interactions in the cosmological dark sector
• Dark Energy in Practice
• MCMC analysis of WMAP3 and SDSS data points to broken symmetry inflaton potentials and provides a lower bound on the tensor to scalar ratio
• Can Astrophysical Gamma Ray Sources Mimic Dark Matter Annihilation in Galactic Satellites?
• Distribution function approach to redshift space distortions. Part II: N-body simulations
• Cross-Correlation of Cosmic Shear and Extragalactic Gamma-ray Background: Constraints on the Dark Matter Annihilation Cross-Section
• Full-Shape Galaxy Power Spectra and the Curvature Tension
• The galaxy power spectrum: precision cosmology from large scale structure?
• Reconstruction of the primordial power spectrum of curvature perturbations using multiple data sets
• Focusing on Warm Dark Matter with Lensed High-redshift Galaxies
• Bar-Halo Friction in Galaxies III: Halo Density Changes
• Stable Higgs Bosons as Cold Dark Matter
• Power spectrum of the maxBCG sample: detection of acoustic oscillations using galaxy clusters
• Are cosmological neutrinos free-streaming?
• Cosmography beyond standard candles and rulers
• Parameterizing the Effect of Dark Energy Perturbations on the Growth of Structures
• Statistical and Systematic Errors in Measurement of Weak-Lensing Minkowski Functionals: Application to Canada-France-Hawaii Lensing Survey
• On Combining Galaxy Clustering and Weak Lensing to Unveil Galaxy Biasing via the Halo Model
• Constraints on Warm Dark Matter models from high-redshift long gamma-ray bursts
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• The Large-Scale 3-point correlation function of SDSS Luminous Red Galaxies
• New interactions in the dark sector mediated by dark energy
• Large Scale Structure Constraints for a Class of f(R) Theories of Gravity
• Dynamics of nonlinear interacting dark energy models
• Distribution function approach to redshift space distortions, Part III: halos and galaxies
• Overcoming the Circular Problem for γ-ray Bursts in Cosmological Global Fitting Analysis
• Model-independent Curvature Determination from Gravitational-Wave Standard Sirens and Cosmic Chronometers
• Isocurvature forecast in the anthropic axion window
• Testing Gravity Using Large-Scale Redshift-Space Distortions
• Reconstructing a general inflationary action
• KiDS+GAMA: Constraints on Horndeski gravity from combined large-scale structure probes
• Constraining $f(R)$ gravity models with disappearing cosmological constant
• Cosmological Constraints on the Modified Entropic Force Model
• EDGE: Two routes to dark matter core formation in ultra-faint dwarfs
• The WiggleZ Dark Energy Survey: measuring the cosmic growth rate with the two-point galaxy correlation function
• Alleviation of Cosmic Age Problem In Interacting Dark Energy Model
• Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
• How clustering dark energy affects matter perturbations
• Gravitational Lensing Simulations I : Covariance Matrices and Halo Catalogues
• Supersonic Relative Velocity Effect on the Baryonic Acoustic Oscillation Measurements
• Large-Scale Structure of the Universe as a Cosmic Standard Ruler
• The Growth of Central and Satellite Galaxies in Cosmological Smoothed Particle Hydrodynamics Simulations
• Testing the Copernican Principle via Cosmological Observations
• Neutrino mass constraint with the Sloan Digital Sky Survey power spectrum of luminous red galaxies and perturbation theory
• The WiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxies
• The expansion field: The value of H_0
• Constraint on the Effective Number of Neutrino Species from the WMAP and SDSS LRG Power Spectra
• Light mass galileons: Cosmological dynamics, mass screening and observational constraints
• Cosmological constraints on neutrino plus axion hot dark matter
• Minimal Supersymmetric Inverse Seesaw: Neutrino masses, lepton flavour violation and LHC phenomenology
• Phenomenology of WIMPy baryogenesis models
• Model-independent estimations for the curvature from standard candles and clocks
• Non-Gaussianities in N-flation
• Dynamics of Quintom and Hessence Energies in Loop Quantum Cosmology
• Cosmological Backreaction from Perturbations
• Holographic f(T)-gravity model with power-law entropy correction
• Constraints on general second-order scalar-tensor models from gravitational Cherenkov radiation
• Reconstructing the Cosmic Expansion History up to Redshift z=6.29 with the Calibrated Gamma-Ray Bursts
• Analytic solution for matter density perturbations in a class of viable cosmological f(R) models
• Growth factor and galaxy bias from future redshift surveys: a study on parametrizations
• Probing elastic interactions in the dark sector and the role of $S_8$
• Dirac Neutrinos with $S_4$ Flavor Symmetry in Warped Extra Dimensions
• Positivity Bounds on Dark Energy: When Matter Matters
• Galaxy-CMB and galaxy-galaxy lensing on large scales: sensitivity to primordial non-Gaussianity
• Analytic study of the effect of dark energy-dark matter interaction on the growth of structures
• Angular Signatures of Annihilating Dark Matter in the Cosmic Gamma-Ray Background
• Holographic Ricci dark energy: Interacting model and cosmological constraints
• Observational Constraints on Kinetic Gravity Braiding from the Integrated Sachs-Wolfe Effect
• Lyman-alpha Forest Constraints on Decaying Dark Matter
• Scale relativity and fractal space-time: theory and applications
• A cosmographic analysis of holographic dark energy models
• Cosmic string parameter constraints and model analysis using small scale Cosmic Microwave Background data
• How to Distinguish Dark Energy and Modified Gravity?
• Voids of dark energy
• Dark Energy and Neutrino Masses from Future Measurements of the Expansion History and Growth of Structure
• Measuring Dark Energy with Gamma-Ray Bursts and Other Cosmological Probes
• Determining Cosmological Parameters with Latest Observational Data
• Bayesian optimal reconstruction of the primordial power spectrum
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• Viability of complex self-interacting scalar field as dark matter
• A Unified Approach to Variational Derivatives of Modified Gravitational Actions
• Spatially Resolved Stellar Kinematics of the Ultra-Diffuse Galaxy Dragonfly 44: II. Constraints on Fuzzy Dark Matter
• Constraining cosmological parameters in FLRW metric with lensed GW+EM signals
• Testing the effect of $H_0$ on $f{\sigma }_8$ tension using a Gaussian Process method
• Future CMB cosmological constraints in a dark coupled universe
• The Universal Einstein Radius Distribution from 10,000 SDSS Clusters
• Attractive Lagrangians for Noncanonical Inflation
• Constraints on f(R) theory and Galileons from the latest data of galaxy redshift surveys
• The Sunyaev-Zel'dovich effects from a cosmological hydrodynamical simulation: large-scale properties and correlation with the soft X-ray signal
• Growth factor parametrization in curved space
• Constraints on Dark Energy from Galaxy Cluster Gas Mass Fraction versus Redshift data
• Dark Matter in a Constrained NMSSM
• Testing power-law cosmology with galaxy clusters
• Constraining dark matter properties with Cosmic Microwave Background observations
• Cosmological constraints on a light non-thermal sterile neutrino
• Systematic effects in the sound horizon scale measurements
• Towards understanding the structure of voids in the cosmic web
• Clustering and redshift-space distortions in interacting dark energy cosmologies
• Reconstructing f(R) theory according to holographic dark energy
• Inferring $S_8(z)$ and $\gamma (z)$ with cosmic growth rate measurements using machine learning
• Cosmological constraints on dark energy in light of gravitational wave bounds
• Mining the SDSS archive. I. Photometric redshifts in the nearby universe
• Hints of Modified Gravity in Cosmos and in the Lab?
• Complete Treatment of Galaxy Two-Point Statistics: Gravitational Lensing Effects and Redshift-Space Distortions
• On the Magnitude of Dark Energy Voids and Overdensities
• Stability of de Sitter spacetime under isotropic perturbations in semiclassical gravity
• How to estimate the 3D power spectrum of the Lyman-$\alpha$ forest
• CFHTLS weak-lensing constraints on the neutrino masses
• UV stable, Lorentz-violating dark energy with transient phantom era
• Non-Gaussianity and large-scale structure in a two-field inflationary model
• Looking Beyond Lambda with the Union Supernova Compilation
• The effects of ellipticity and substructure on estimates of cluster density profiles based on lensing and kinematics
• 3D Genus Topology of Luminous Red Galaxies
• Contiguous redshift parameterizations of the growth index
• Chasing the non-linear evolution of matter power spectrum with numerical resummation method: solution of closure equations
• Apparent and average acceleration of the Universe
• Angular correlation function of 1.5 million LRGs: clustering evolution and a search for BAO
• Cross-correlating WMAP5 with 1.5 million LRGs: a new test for the ISW effect
• Dark energy: investigation and modeling
• A Millimetre Survey of Starburst Dominated Ultraluminous Infrared Galaxies at z~2
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• On the signature of $z\sim 0.6$ superclusters and voids in the Integrated Sachs-Wolfe effect
• Scale-dependent halo bias from scale-dependent growth
• The Sloan Digital Sky Survey Quasar Lens Search. IV. Statistical Lens Sample from the Fifth Data Release
• Magnification-Temperature Correlation: the Dark Side of ISW Measurements
• Background history and cosmic perturbations for a general system of self-conserved dynamical dark energy and matter
• Effects of cosmological model assumptions on galaxy redshift survey measurements
• Dark energy from primordial inflationary quantum fluctuations
• Searching for Inflation in Simple String Theory Models: An Astrophysical Perspective
• Mapping the allowed parameter space for decaying dark matter models
• Non-vacuum Solutions of Bianchi Type VI_0 Universe in f(R) Gravity
• An extensive investigation of the Generalised Dark Matter model
• What is the best way to measure baryonic acoustic oscillations?
• Connecting the primordial and Galactic deuterium abundances
• Observational Constraints on Modified Chaplygin Gas from Cosmic Growth
• Constraint on the cosmological f(R) model from the multipole power spectrum of the SDSS luminous red galaxy sample and prospects for a future redshift survey
• On the determination of curvature and dynamical Dark Energy
• The growth of linear perturbations in the DGP model
• How robust are inflation model and dark matter constraints from cosmological data?
• Cosmological perturbations and observational constraints on nonlocal massive gravity
• Galaxy power spectrum in redshift space: combining perturbation theory with the halo model
• Dark-matter decays and Milky Way satellite galaxies
• Entropic cosmology in a dissipative universe
• Interacting Cosmological Fluids and the Coincidence Problem
• Eddington-Born-Infeld cosmology: a cosmographic approach, a tale of doomsdays and the fate of bound structures
• Nongaussianity from Particle Production During Inflation
• Anisotropic cosmological solutions in massive vector theories
• Machine Learning the Cosmic Curvature in a Model-independent Way
• WMAP 3-year primordial power spectrum
• The growth index of matter perturbations and modified gravity
• A search for a dark matter annihilation signal towards the Canis Major overdensity with H.E.S.S
• Tuning Hyperparameters without Grad Students: Scalable and Robust Bayesian Optimisation with Dragonfly
• New constraints on the observable inflaton potential from WMAP and SDSS
• Cosmological Constraints on Decaying Dark Matter
• Constraints on growth index parameters from current and future observations
• Ambiguous Tests of General Relativity on Cosmological Scales
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• New constraints on the linear growth rate using cosmic voids in the SDSS DR12 datasets
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• A Testable Solution of the Cosmological Constant and Coincidence Problems
• Unified Dark Matter models with fast transition
• Holographic dark matter and dark energy with second order invariants
• Neutrino mass from future high redshift galaxy surveys: sensitivity and detection threshold
• Cosmological observations in a modified theory of gravity (MOG)
• Anti-deuterons from heavy Dark Matter
• Regarding the Line-of-Sight Baryonic Acoustic Feature in the Sloan Digital Sky Survey and Baryon Oscillation Spectroscopic Survey Luminous Red Galaxy Samples
• Tension in the Recent Type Ia Supernovae Datasets
• Testing the DGP model with ESSENCE
• Velocity bias in the distribution of dark matter halos
• Cosmological implications and structure formation from a time varying vacuum
• Revisiting the Cosmological Constraints on the Interacting Dark Energy Models
• Bayesian Evidence for a Cosmological Constant using new High-Redshift Supernovae Data
• Modified Holographic Dark Energy
• A step towards testing general relativity using weak gravitational lensing and redshift surveys
• What do WMAP and SDSS really tell about inflation?
• The effect of massive neutrinos on the Sunyaev-Zeldovich and X-ray observables of galaxy clusters
• Toward a Unified Description of Dark Energy and Dark Matter from the Abnormally Weighting Energy Hypothesis
• An effective description of dark matter and dark energy in the mildly non-linear regime
• Growth of matter perturbations in clustered holographic dark energy cosmologies
• How to generate a significant effective temperature for cold dark matter, from first principles
• Backreaction from non-conformal quantum fields in de Sitter spacetime
• How Late can the Dark Matter form in our universe?
• Dark Matter Gravitational Clustering With a Long-Range Scalar Interaction
• Cosmology in scalar-vector-tensor theories
• A parametrization for the growth index of linear matter perturbations
• Exploring the Systematic Uncertainties of Type Ia Supernovae as Cosmological Probes
• Tight constraints on F- and D-term hybrid inflation scenarios
• Luminous Red Galaxy Halo Density Field Reconstruction and Application to Large Scale Structure Measurements
• 2-FAST: Fast and accurate computation of projected two-point functions
• Discriminating dark matter candidates using direct detection
• Unified Dark Matter scalar field models with fast transition
• Adjoint SUSY $SU(5)$ Grand Unified Model with $S_4$ Flavor Symmetry
• Cold Dark Matter Isocurvature Perturbations: Constraints and Model Selection
• Cosmological perturbations in an effective and genuinely phantom dark energy Universe
• A new perspective on the relation between dark energy perturbations and the late-time ISW effect
• Exploring compressed supersymmetry with same-sign top quarks at the Large Hadron Collider
• Power-law cosmology, SN Ia, and BAO
• Cosmological CPT Violation, Baryon/Leptogenesis and CMB Polarization
• Cosmic Magnetism in Centimeter and Meter Wavelength Radio Astronomy
• DIVE in the cosmic web: voids with Delaunay Triangulation from discrete matter tracer distributions
• QCD ghost f(T)-gravity model
• Testing Einstein's gravity and dark energy with growth of matter perturbations: Indications for new Physics?
• The REFLEX II galaxy cluster survey: power spectrum analysis
• A See-Saw $S_4$ model for fermion masses and mixings
• Limits on coupling between dark components
• Model-independent Distance Calibration and Curvature Measurement using Quasars and Cosmic Chronometers
• Combining perturbation theories with halo models for the matter bispectrum
• Testing cold dark matter with the low mass Tully-Fisher relation
• Observational constraints on cosmic neutrinos and dark energy revisited
• Towards a self-consistent analysis of the anisotropic galaxy two- and three-point correlation functions on large scales: application to mock galaxy catalogues
• Dynamics of holographic vacuum energy in the DGP model
• Observational biases in Lagrangian reconstructions of cosmic velocity fields
• Cosmic age, Statefinder and $Om$ diagnostics in the decaying vacuum cosmology
• On the nature of dark energy: the lattice Universe
• Confronting dark energy models mimicking $\Lambda$CDM epoch with observational constraints: future cosmological perturbations decay or future Rip?
• Primordial Tensor Perturbation in Double Inflationary Scenario with a Break
• The Clustering and Host Halos of Galaxy Mergers at High Redshift
• Incompatibility of Rotation Curves with Gravitational Lensing for TeVeS
• Graviton mass might reduce tension between early and late time cosmological data
• Coupled quintessence and vacuum decay
• The full Fisher matrix for galaxy surveys
• Constraining An Exact Brans-Dicke gravity theory with Recent Observations
• The Angular Power Spectra of Photometric SDSS LRGs
• The Rapidly Flaring Afterglow of the Very Bright and Energetic GRB 070125
• Dark energy, gravitation and supernovae
• Cosmic Constraint to DGP Brane Model: Geometrical and Dynamical Perspectives
• Observational tests for Λ(t)CDM cosmology
• A New Statistic for Analyzing Baryon Acoustic Oscillations
• The growth factor of matter perturbations in an f(R) gravity
• CosmoBit: A GAMBIT module for computing cosmological observables and likelihoods
• Constraining Inflation
• Cosmological constraints on general, single field inflation
• Neutrino masses from clustering of red and blue galaxies: a test of astrophysical uncertainties
• Statistical analysis of galaxy surveys - III: The non-linear clustering of red and blue galaxies in the 2dFGRS
• Searching for scalar gravitational interactions in current and future cosmological data
• Dynamical Constraints on the Local Group from the CMB and 2MRS Dipoles
• Multiple kinetic k-essence, phantom barrier crossing and stability
• The imprint of $f(R)$ gravity on weak gravitational lensing II : Information content in cosmic shear statistics
• Constraining DGP Gravity from Observational Data
• Measuring the reionization optical depth without large-scale CMB polarization
• Galaxy Clustering Analysis with SimBIG and the Wavelet Scattering Transform
• Impact of anisotropic stress of free-streaming particles on gravitational waves induced by cosmological density perturbations
• Testing for dynamical dark energy models with redshift-space distortions
• Polytropic dark matter flows illuminate dark energy and accelerated expansion
• Expansion schemes for gravitational clustering: computing two-point and three-point functions
• Perturbations of ultralight vector field dark matter
• Cosmological Avatars of the Landscape II: CMB and LSS Signatures
• WMAP 5-year constraints on lepton asymmetry and radiation energy density: Implications for Planck
• Light propagation in inhomogeneous and anisotropic cosmologies
• Mixed Sneutrinos, Dark Matter and the LHC
• Cosmological Studies with Radio Galaxies and Supernovae
• How to Falsify the GR+LambdaCDM Model with Galaxy Redshift Surveys
• Computing the Small-Scale Galaxy Power Spectrum and Bispectrum in Configuration-Space
• Weak lensing induced by second-order vector mode
• Strongly Coupled Dark Energy Cosmologies: preserving LCDM success and easing low scale problems II - Cosmological simulations
• Measuring large-scale structure with quasars in narrow-band filter surveys
• Initial Conditions for Non-Canonical Inflation
• Precision measurements, dark matter direct detection and LHC Higgs searches in a constrained NMSSM
• Probing Dark Energy Dynamics from Current and Future Cosmological Observations
• Reconstructing the potentials for the quintessence and tachyon dark energy, from the holographic principle
• Signatures of clumpy dark matter in the global 21 cm background signal
• "Detuned" f(R) gravity and dark energy
• Test of the FLRW metric and curvature with strong lens time delays
• Is the Dynamics of Tracking Dark Energy Detectable?
• The homogeneity scale and the growth rate of cosmic structures
• Modifications by QCD transition and $e^{+}{e}^{-}$ annihilation on analytic spectrum of relic gravitational waves in accelerating universe
• Gravitational quantum effects on power spectra and spectral indices with higher-order corrections
• WIMPy Leptogenesis With Absorptive Final State Interactions
• How does non-linear dynamics affect the baryon acoustic oscillation?
• Constraints on Neutrino Mass and Light Degrees of Freedom in Extended Cosmological Parameter Spaces
• Cosmological Constraints on Variable Warm Dark Matter
• Reconstruction of interacting dark energy models from parameterizations
• Luminous Red Galaxy Clustering at z~0.7 - First Results using AAOmega
• Weak gravitational lensing effects on cosmological parameters and dark energy from gamma-ray bursts
• Detecting relics of a thermal gravitational wave background in the early Universe
• Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids
• Nonlinear corrections to the cosmological matter power spectrum and scale-dependent galaxy bias: implications for parameter estimation
• Large-scale growth evolution in the Szekeres inhomogeneous cosmological models with comparison to growth data
• Observational Tests of Gauss-Bonnet Like Dark Energy Model
• Three-Point Correlations in f(R) Models of Gravity
• Curvature from strong gravitational lensing: a spatially closed Universe or systematics?
• Exploring the Hubble Tension and Spatial Curvature from the Ages of Old Astrophysical Objects
• A comparison of the galaxy peculiar velocity field with the PSCz gravity field-- A Bayesian hyper-parameter method
• Testing modified gravity models with recent cosmological observations
• Spectroscopic Confirmation of the Fifth Image of SDSS J1004+4112 and Implications for the M_BH-sigma_* Relation at z=0.68
• Galaxy and Mass Assembly (GAMA): Colour and luminosity dependent clustering from calibrated photometric redshifts
• WMAP5 and the Cluster Mass Function
• Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying $\beta$ and different light-curve fitters
• Anisotropies in the Diffuse Gamma-Ray Background from Dark Matter with Fermi LAT: a closer look
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• Forecasting the Dark Energy Measurement with Baryon Acoustic Oscillations: Prospects for the LAMOST surveys
• Stealth Acceleration and Modified Gravity
• Cosmological data analysis of f(R) gravity models
• Constraining power of cosmological observables: blind redshift spots and optimal ranges
• The imprint of $f(R)$ gravity on weak gravitational lensing I: Connection between observables and large scale structure
• Query Efficient Posterior Estimation in Scientific Experiments via Bayesian Active Learning
• The Metric of the Cosmos from Luminosity and Age Data
• Big Bang nucleosynthesis in scalar tensor gravity: the key problem of the ${}^7$Li abundance
• Characteristic Scales of Baryon Acoustic Oscillations from Perturbation Theory: Non-linearity and Redshift-Space Distortion Effects
• Constraints on the Primordial Magnetic Field from ${\sigma }_8$
• DBI N-flation
• Reconstruction of new holographic scalar field models of dark energy in Brans-Dicke Universe
• The dynamical viability of scalar-tensor gravity theories
• The Influence of Galaxy Formation Physics on Weak Lensing Tests of General Relativity
• Non-Gaussian errors of baryonic acoustic oscillations
• Systematics of multi-field effects at the end of warped brane inflation
• Cosmological Models and Latest Observational Data
• Cosmology and thermodynamics of FRW universe with bulk viscous stiff fluid
• A Radial Measurement of the Galaxy Tidal Alignment Magnitude with BOSS Data
• The $\Lambda$CDM growth rate of structure revisited
• Scalars, Vectors and Tensors from Metric-Affine Gravity
• DM haloes in the fifth-force cosmology
• Determining neutrino properties using future galaxy redshift surveys
• Redshift space power spectrum beyond Einstein-de Sitter kernels
• A new method for the determination of the growth rate from galaxy redshift surveys
• Detecting the power spectrum turnover with HI intensity mapping
• An improved model of redshift-space distortions around voids: application to quintessence dark energy
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• Estimating the amount of vorticity generated by cosmological perturbations in the early universe
• Improved estimation of cluster mass profiles from the cosmic microwave background
• Model independent constraints on mass-varying neutrino scenarios
• Covariance matrices for halo number counts and correlation functions
• Galaxy peculiar velocities and evolution-bias
• Model-independent Estimations for the Cosmic Curvature from the Latest Strong Gravitational Lensing Systems
• Changes in the halo formation rates due to features in the primordial spectrum
• Non-parametric Dark Energy Degeneracies
• Cosmological Parameters from the QUaD CMB polarization experiment
• Anisotropies in the Cosmic Neutrino Background after WMAP 5-year Data
• How to constrain inflationary parameter space with minimal priors
• Bayesian Model Averaging in Astrophysics: A Review
• High-resolution temporal constraints on the dynamics of dark energy
• Confronting MOND and TeVeS with strong gravitational lensing over galactic scales: an extended survey
• Cosmic microwave background and large-scale structure constraints on a simple quintessential inflation model
• A conventional approach to the dark-energy concept
• Cosmography and large scale structure by f(R) gravity: new results
• Mass of Galactic Lenses in Modified Newtonian Dynamics
• Probing for the Cosmological Parameters with PLANCK Measurement
• Cosmological dark energy effects from entanglement
• Semi-shifted hybrid inflation with B-L cosmic strings
• Cosmic strings interacting with dark strings
• AGN and QSOs in the eROSITA All-Sky Survey -- Part II: The large-scale structure
• Dark Energy: The Shadowy Reflection of Dark Matter?
• Constraints on cosmic curvature with lensing time delays and gravitational waves
• Primordial Magnetic Field Effects on the CMB and Large Scale Structure
• Increasing the Fisher Information Content in the Matter Power Spectrum by Non-linear Wavelet Weiner Filtering
• A Dark Matter Candidate from an Extra (Non-Universal) Dimension
• Sequestering the Gravitino: Neutralino Dark Matter in Gauge Mediation
• Constraining Cosmological Parameters with Observational Data Including Weak Lensing Effects
• Gaugessence: a dark energy model with early time radiation-like equation of state
• Should we doubt the cosmological constant?
• A detection of baryon acoustic oscillations from the distribution of galaxy clusters
• Running vacuum in Brans-Dicke theory: a possible cure for the ${\sigma }_8$ and $H_0$ tensions
• On the origin of the helium-rich population in Omega Centauri
• On the growth of perturbations in interacting dark energy and dark matter fluids
• Special Relativity induced by Granular Space
• Goldilocks Supersymmetry: Simultaneous Solution to the Dark Matter and Flavor Problems of Supersymmetry
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• Anisotropic solid dark energy
• Testing Oscillating Primordial Spectrum and Oscillating Dark Energy with Astronomical Observations
• Constraints on neutrino masses from WMAP5 and BBN in the lepton asymmetric universe
• A dynamical system representation of generalized Rastall gravity
• Euclid preparation. XLI. Galaxy power spectrum modelling in real space
• Angular Power Spectra with Finite Counts
• Interacting Dark Energy: Decay into Fermions
• Non-Gaussian Error in Galaxy Survey (Part 1)
• Clustering dark energy imprints on cosmological observables of the gravitational field
• Neutrino mass from cosmology: Impact of high-accuracy measurement of the Hubble constant
• Observational constraints on a generalized equation of state model
• Could multiple voids explain the Cosmic Microwave Background Cold Spot anomaly?
• Constraints on the neutrino mass and the primordial magnetic field from the matter density fluctuation parameter ${\sigma }_8$
• Topology of large scale structure as test of modified gravity
• Dark matter in minimal supergravity with type-II seesaw
• Reduced modified Chaplygin gas cosmology
• Toward Accurate Modeling of the Nonlinear Matter Bispectrum: Standard Perturbation Theory and Transients from Initial Conditions
• Cosmology with Phase Statistics: Parameter Forecasts and Detectability of BAO
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Cosmological acceleration
• Density preturbations in a finite scale factor singularity universe
• Investigations of the Non-Linear LMC Cepheid Period-Luminosity Relation with Testimator and Schwarz Information Criterion Methods
• Cosmological Constraints on Dissipative Models of Inflation
• The growth of matter perturbations in the f(T) gravity
• A Faster Fourier Transform? Computing Small-Scale Power Spectra and Bispectra for Cosmological Simulations in $\mathcal{O}(N^2)$ Time
• Observations of the Prompt Gamma-Ray Emission of GRB 070125
• Reconstructing f(R) Gravity from a Chaplygin Scalar Field in de Sitter Spacetimes
• Using Big Bang Nucleosynthesis to Extend CMB Probes of Neutrino Physics
• An explanation for dark matter and dark energy consistent with the Standard Model of particle physics and General Relativity
• Enhanced Inflation in the Dirac-Born-Infeld framework
• Anisotropic $k$-essence
• Redshift-space distortions from the cross-correlation of photometric populations
• The effect of dark strings on semilocal strings
• Lensing reconstruction of cluster-mass cross-correlation with cosmic microwave background polarization
• Extending Recovery of the Primordial Matter Power Spectrum
• Probing the nature of cosmic acceleration
• GCG Parametrization for Growth Function and Current Constraints
• Age Problem in Lemaitre-Tolman-Bondi Void Models
• Weakly-Gravitating Objects in dynamical Chern-Simons gravity and Constraints with Gravity Probe B
• Decomposition of Spectra from Redshift Distortion Maps
• Evolution of the curvature perturbation during and after multi-field inflation
• Ghosts in asymmetric brane gravity and the decoupled stealth limit
• Cosmological constraints on polytropic gas model
• New method to constrain the relativistic free-streaming gas in the Universe
• Using Lagrangian perturbation theory for precision cosmology
• Constraints on running vacuum model with $H(z)$ and $f{\sigma }_8$
• On the consistency of tachyon warm inflation with viscous pressure
• Constraining Dark Matter Properties with Gamma-Rays from the Galactic Center with Fermi-LAT
• Ballistic Dark Matter oscillates above $\Lambda$CDM
• Constraints on Dark Energy Parameters from Correlations of CMB with LSS
• Efficient parallel algorithm for estimating higher-order polyspectra
• Probing Primordial Non-Gaussianity with Weak Lensing Minkowski Functionals
• Growth of perturbations in dark energy parametrization scenarios
• From model dynamics to oscillating dark energy parameterisation
• Wavelet analysis of baryon acoustic structures in the galaxy distribution
• Effect of model-dependent covariance matrix for studying Baryon Acoustic Oscillations
• Radiative stability and observational constraints on dark energy and modified gravity
• Lensing as a Probe of Early Universe: from CMB to Galaxies
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The matter density and baryon fraction from the galaxy power spectrum at redshift $0.6<z<1.1$
• Dynamics and constraints of the dissipative Liouville cosmology
• Dynamics and Constraints of the Massive Gravitons Dark Matter Flat Cosmologies
• Beyond the growth rate of cosmic structure: Testing modified gravity models with an extra degree of freedom
• Matter power spectra in dynamical-Dark Energy cosmologies
• Neutrino Mass Inference from SZ Surveys
• Dark Matter from the Inflaton Field
• Late-time acceleration and inflation in a Poincaré gauge cosmological model
• Broadband Alcock-Paczynski test exploiting redshift distortions
• Detecting Baryon Acoustic Oscillations
• The VIMOS VLT Deep Survey: Testing the gravitational instability paradigm at z ~ 1
• Direct Search for Dark Matter - Striking the Balance - and the Future
• Interacting dark energy: generic cosmological evolution for two scalar fields
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• Cosmological Information Contents on the Light-Cone
• Viscous Self Interacting Dark Matter Cosmology For Small Redshift
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• Properties of the exact analytic solution of the growth factor and its applications
• The effects of the small-scale behaviour of dark matter power spectrum on CMB spectral distortion
• Flat Tree-level Inflationary Potentials in Light of CMB and LSS Data
• Delayed Recombination and Standard Rulers
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Emergent Universe in the Braneworld Scenario
• Reconstruction of halo power spectrum from redshift-space galaxy distribution: cylinder-grouping method and halo exclusion effect
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Distance Probes of Dark Energy
• Constraining the Milky Way Dark Matter Density Profile with Gamma-Rays with Fermi-LAT
• Constraints on Dark Energy Models Using Late Universe Probes
• A Dark Energy Model in Lyra Manifold
• Validity of Generalized Second Law of Thermodynamics in the Logamediate and Intermediate scenarios of the Universe
• Constraining warm dark matter mass with cosmic reionization and gravitational wave
• The Imprint of Cosmic Reionization on Galaxy Clustering
• Observing trans-Planckian ripples in the primordial power spectrum with future large scale structure probes
• Real space tests of the statistical isotropy and Gaussianity of the WMAP CMB data
• Reconciling the cosmic age problem in the R_h=ct Universe
• Dynamics of interacting scalar field model in the realm of chiral cosmology
• Late time acceleration in a slow moving galileon field
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• The Integrated Sachs-Wolfe Effect in Time Varying Vacuum Model
• The lessons from the running of the tensor-to-scalar ratio
• The Impact of Prior Assumptions on Bayesian Estimates of Inflation Parameters and the Expected Gravitational Waves Signal from Inflation
• Mass assembly history and infall time of the Fornax dwarf spheroidal galaxy
• Supernova, baryon acoustic oscillations, and CMB surface distance constraints on f(G) higher order gravity models
• Nontrivial Geometries: Bounds on the Curvature of the Universe
• Does Planck mass run on the cosmological horizon scale?
• Tetrad formalism for exact cosmological observables
• Systematics in the Gamma Ray Bursts Hubble diagram
• Probing Dark Energy with the Kunlun Dark Universe Survey Telescope
• Baryonic matter perturbations in decaying vacuum cosmology
• The dark side of curvature
• Interacting holographic Ricci dark energy as running vacuum
• The Hubble constant and dark energy from cosmological distance measures
• Second-order matter fluctuations via higher-order galaxy correlators
• How the curvaton scenario, modulated reheating and an inhomogeneous end of inflation are related
• Mass-varying neutrino in light of cosmic microwave background and weak lensing
• Dynamic analysis of noncanonical warm inflation
• Analytical Gaussian Process Cosmography: Unveiling Insights into Matter-Energy Density Parameter at Present
• Constraints on Generalized Dark Energy from Recent Observations
• Joint constraints on reionization: a framework for combining the global 21cm signal and the kinetic Sunyaev-Zel'dovich effect
• Information Content in the Angular Power Spectrum of Weak Lensing: Wavelet Method
• Non-sphericity of ultralight axion dark matter haloes in the Galactic dwarf spheroidal galaxies
• Relaxing the Cosmological Constraints on Unparticle Dark Component
• Anisotropic Extinction Distortion of the Galaxy Correlation Function
• Dark Energy Cosmology with the Alternative Cosmic Microwave Background Data
• Constraints on Models with a Break in the Primordial Power Spectrum
• Gauge conditions in combined dark energy and dark matter systems
• Non-Perturbative Yang-Mills Condensate as Dark Energy
• Natural scaling for dark energy
• Prospects in Constraining the Dark Energy Potential
• Structure Formation in Various Dynamical Dark Energy Scenarios
• Conformally and Disformally Coupled Vector field Models of Dark Energy
• The cosmology of $f(R,L_m)$ gravity: constraining the background and perturbed dynamics
• Halting eternal acceleration with an effective negative cosmological constant
• Likelihood of the Power Spectrum in Cosmological Parameter Estimation
• Neutrino Dark Energy With More Than One Neutrino Species
• CMB anisotropies from acausal scaling seeds
• Emergent Cosmos in Einstein-Cartan Theory
• Cosmological constraints on $\gamma$-gravity models
• Testing DM halos using rotation curves and lensing: A warning on the determination of the halo mass
• Relaxing neutrino mass bounds by a running cosmological constant
• Is dark energy from cosmic Hawking radiation?
• Designing Decisive Detections
• Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
• Damping of the baryon acoustic oscillations in the matter power spectrum as a probe of the growth factor
• Testing the statistical isotropy of large scale structure with multipole vectors
• Quantum Statistical Entropy and Minimal Length of 5D Ricci-flat Black String with Generalized Uncertainty Principle
• An original constraint on the Hubble constant: h>0.74
• Cosmic Bose dark matter
• Constraints on primordial non-Gaussianity from WMAP7 and Luminous Red Galaxies power spectrum and forecast for future surveys
• A thermodynamic point of view on dark energy models
• Covariance of dark energy parameters and sound speed constraints from large HI surveys
• Holographic Λ(t)CDM model in a non-flat universe
• Current cosmological constraints on the curvature, dark energy and modified gravity
• Viscous extended holographic Ricci dark energy in the framework of standard Eckart theory
• EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf
• Cosmological effects of coupled dark matter
• Constraining dark matter sub-structure with the dynamics of astrophysical systems
• Testing a Phenomenologically Extended DGP Model with Upcoming Weak Lensing Surveys
• Improved parametrization of the growth index for dark energy and DGP models
• Effects on the two-point correlation function from the coupling of quintessence to dark matter
• Viable dark energy models using pseudo-Nambu-Goldstone bosons
• Higher-order gravity in higher dimensions: Geometrical origins of four-dimensional cosmology?
• Skewness as a probe of Baryon Acoustic Oscillations
• Perturbation level interacting dark energy model and its consequence on late-time cosmological parameters
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• Growth of matter fluctuations in $f(R,T)$ Gravity
• First and second order cosmological perturbations in light mass Galileon models
• Simultaneous effect of Modified Gravity and Primordial Non-Gaussianity in Large Scale Structure Observations
• Age problem in holographic dark energy
• Running vacuum model in non-flat universe
• Discriminating Electroweak-ino Parameter Ordering at the LHC and Its Impact on LFV Studies
• Magnetic Field of a Compact Spherical Star under f(R,T) Gravity
• Gravitational Lensing Effects on the Baryonic Acoustic Oscillation Signature in the Redshift-Space Correlation Function
• Non-Gaussian error bars in galaxy surveys -- II
• The cluster-galaxy cross-spectrum: an additional probe of cosmological and halo parameters
• The Fate of the Universe: Dark Energy Dilution?
• Global neutrino parameter estimation using Markov Chain Monte Carlo
• Mass Limits on Neutralino Dark Matter
• Fast analytical calculation of the random pair counts for realistic survey geometry
• Evolution of dissipative and non-dissipative universes in holographic cosmological models with a power-law term
• Modelling ultra-fine structure in dark matter halos
• Slow-rotating charged black hole solution in dynamical Chern-Simons modified gravity
• Constraints on scalar-tensor theories of gravity from observations
• Constraints on the multi-lognormal magnetic fields from the observations of the cosmic microwave background and the matter power spectrum
• Stability of the holographic description of the Universe
• CMB Spectral $\mu$-Distortion of Multiple Inflation Scenario
• Neutrino mass hierarchy and the origin of leptonic flavor mixing from the right-handed sector
• Cosmological implications of different baryon acoustic oscillation data
• Selecting samples of galaxies with fewer Fingers-of-God
• Einstein Static Universe and its Stability in Generalized Rastall Gravity
• Universal subhalo accretion in cold and warm dark matter cosmologies
• Cosmology of fermionic dark matter
• Constraining Decaying Dark Matter
• Ultra-fine dark matter structure in the Solar neighbourhood
• Impact of a Warm Dark Matter late-time velocity dispersion on large-scale structures
• Expansion and Growth of Structure Observables in a Macroscopic Gravity Averaged Universe
• Towards an Observational Appraisal of String Cosmology
• On tachyonic stability priors for dark energy
• Towards a warped inflationary brane scanning
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• Keeping It Real: Revisiting a Real-Space Approach to Running Ensembles of Cosmological N-body Simulations
• The Cosmology of Asymmetric Brane Modified Gravity
• The measurements of matter density perturbations amplitude from cosmological data
• Ghost Dark Matter
• Improvements in the X-ray luminosity function and constraints on the Cosmological parameters from X-ray luminous clusters
• Cosmological implications of the KATRIN experiment
• A minimal set of invariants as a systematic approach to higher order gravity models: Physical and Cosmological Constraints
• The DAMIC-M Low Background Chamber
• On the Effective Equation of State of Dark Energy
• Structure formation in clustering DBI dark energy model with constant sound speed
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• Probing for cosmological parameters with LAMOST measurement
• Unraveling the nature of Gravity through our clumpy Universe
• Gravitational instability of the primordial plasma: anisotropic evolution of structure seeds
• Cosmological constant constraints from observation-derived energy condition bounds and their application to bimetric massive gravity
• Geometrical tests of cosmological models. I. Probing dark energy using the kinematics of high-redshift galaxies
• Slow-roll reconstruction for running spectral index
• Holographic dark information energy: Predicted dark energy measurement
• Testing for Features in the Primordial Power Spectrum
• Cosmic constraint on the unified model of dark sectors with or without a cosmic string fluid in the varying gravitational constant theory
• Cosmic Growth Signatures of Modified Gravitational Strength
• Constraining dark energy using observational growth rate data
• Chaplygin gas in decelerating DGP gravity and the age of the oldest star
• The potential of advanced ground-based gravitational wave detectors to detect generic deviations from general relativity
• Constraining Slow-Roll Inflation in the Presence of Dynamical Dark Energy
• Reconstructing the parameter space of non-analytical cosmological fixed points
• On the Determination of Neutrino Masses and Dark Energy Evolution from the Cross Correlation of CMB and LSS
• Bayesian Multi-line Intensity Mapping
• A comprehensive data-driven odyssey to explore the equation of state of dark energy
• The Matrix Reloaded - on the Dark Energy Seesaw
• Warm Hawking Relics From Primordial Black Hole Domination
• Constraining Neutrinos and Dark Energy with Galaxy Clustering in the Dark Energy Survey
• Augmenting photometric redshift estimates using spectroscopic nearest neighbours
• Weak gravitational lensing as a probe of physical properties of substructures in dark matter halos
• Observable cosmological vector mode in the dark ages
• Cosmological consequences of Modified Gravity (MOG)
• Bayesian analysis of running holographic Ricci dark energy
• A Well-Behaved f(R) Gravity Model in Planetary Motions
• Second order invariants and holography
• Impact of lensing magnification on the analysis of galaxy clustering in redshift space
• Birth of the Universe from the Multiverse, MG13
• Brane cosmology from observational surveys and its comparison with standard FRW cosmology
• Quantum fields near phantom-energy `sudden' singularities
• Expressing the equation of state parameter in terms of the three dimensional cosmic shear
• Bianchi type I models with two tilted fluids
• Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
• Conditions for the Absence of Infrared Sensitivity in Cosmological Probes in Any Gravity Theories
• Holographic Bound in Quantum Field Energy Density and Cosmological Constant
• Parameters and pitfalls in dark energy models with time varying equation of state
• Impact of dark energy on the equation of state in light of the latest cosmological data
• Role of Future SNIa Data from Rubin LSST in Reinvestigating Cosmological Models
• Incompatibility of Standard Galaxy Bias Models in General Relativity
• Confronting the damping of the baryon acoustic oscillations with observation
• Primordial Non-Gaussianity from LAMOST Surveys
• Determining accurate measurements of the growth rate from the galaxy correlation function in simulations
• SUSY SU(5) $\times S_4$ GUT Flavor Model for Fermion Masses and Mixings with Adjoint, Large ${\theta }_{13}^{PMNS}$
• Constraints on dark energy evolution
• Bigravitational inflation
• Simulating the collapse of rotating primordial gas clouds to study the survival possibility of Pop III protostars
• Red Giant evolution in Modified Gravity
• Bias-Limited Extraction of Cosmological Parameters
• Direct WIMP identification: Physics performance of a segmented noble-liquid target immersed in a Gd-doped water veto
• Searching for non-diagonal Mass varying mechanism in the ${\nu }_{\mu }$-${\nu }_{\tau }$ system
• Modified gravity with disappearing cosmological constant
• Observational constraints on a Yang-Mills condensate dark energy model
• CMB and LSS constraints on a single-field model of inflation
• Optimizing the Recovery of Fisher Information in the Dark Matter Power Spectrum
• A method to extract the redshift distortions beta parameter in configuration space from minimal cosmological assumptions
• Knotted strings and leptonic flavor structure
• Reconstruction of energy conditions from observations and implications for extended theories of gravity
• Constraints on the Neutrino Mass from SZ Surveys
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• Unification of Dark Matter and Dark Energy in a Modified Entropic Force Model
• Probing the shape and internal structure of dark matter halos with the halo-shear-shear three-point correlation function
• Modelling the environmental dependence of the growth rate
• Mass Varying Neutrinos in Supernovae
• Effects of high-order operators in non-relativistic Lifshitz holography
• N=2 PNGB Quintessence Dark Energy
• Collider Physics and Cosmology
• Quantum Yang-Mills Condensate Dark Energy Models
• Large-scale structure power spectrum from scalar-tensor gravity
• Perturbations of Dark Matter Gravity
• Bayesian inference methodology for Primordial Power Spectrum reconstructions from Large Scale Structure
• Can MONDian vector theories explain the cosmic speed up ?
• An Improved Photometric Calibration of the Sloan Digital Sky Survey Imaging Data
• Cosmology with Galaxy Correlations
• Constants of extended Standard Model and search for their temporal variations
• A New Approach to Testing Dark Energy Models by Observations
• Direct Determination of Expansion History Using Redshift Distortions
• Data-driven Cosmology from Three-dimensional Light Cones
• Eternally inflating cosmologies from intersecting spacelike branes
• Comment on "The Real Problem with MOND" by Scott Dodelson, arXiv:1112.1320
• Radiation Driven Inflation
• Constraining disformal couplings with Redshift Space Distortion
• Large-scale structure formation in cosmology with classical and tachyonic scalar fields
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• Role of Spatial Curvature in a Dark Energy Interacting Model
• Axion hot dark matter bounds
• Comparison of Strong Gravitational Lens Model Software I. Time delay and mass calculations are sensitive to changes in redshift and are model dependent
• Non-adiabatic instability in coupled dark sectors
• Glass-Like Random Catalogues for Two-Point Estimates on the Light Cone
• Reconstructing the velocity field beyond the local universe
• How to Measure the Cosmic Curvature
• PAC Best Arm Identification Under a Deadline
• Accelerating BAO Scale Fitting Using Taylor Series
• The Power Spectrum of Cosmological Number Densities
• Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters
• Merging Rates of the First Objects and the Formation of First Mini-Filaments in Models with Massive Neutrinos
• Cosmological implications of electromagnetically interacting dark matter: milli-charged particles and atoms with singly and doubly charged dark matter
• Precision Cosmology and the Landscape
• The Effects of Spatial Curvature on Cosmic Evolution
• 21-cm power spectrum and ionization bias as a probe of long-mode modulated non Gaussian sky
• Observations of General Relativity at strong and weak limits
• Spinor-Unit Field Representation of Electromagnetism Applied to a Model Inflationary Cosmology
• A Null Test of the Metric Nature of the Cosmic Acceleration
• Stability of S-brane singular solutions and expansion of the universe
• Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales
• Evolution of entropic dark energy and its phantom nature
• Holographic dark energy in Einstein-Cartan spin cosmology
• Redshift-space distortion from dynamical dark energy with time-dependent Lagrangian perturbation theory
• Possible consistent extra time dimensions in the early universe
• The evolution of universe in the two-scalar theory
• Flavour Condensate and the Dark Sector of the Universe
• Coupling dark-baryonic matter density profile for vacuum decay scenarios
• Effective dark energy from decoherence
• Skewness as a Probe of Gravity: Real and Redshift Space Counts-In-Cells
• Determining the expansion history of the universe with the three dimensional cosmic shear
• Non-Gaussianity in the Squeezed Three-Point Correlation from the Relativistic Effects
• Testing the growth of cosmic structures during the Dark Ages
• Manifestations of String Theory in Astrophysical Data and at the LHC
• Cosmic Dipoles from Large-Scale Structure Surveys
• Running vacuum model versus $\Lambda$CDM -- a Bayesian analysis
• Expansion series of the pairwise velocity generating function and its implications on redshift space distortion modeling
• Dark Energy Effects on Charged and Rotating Black Holes
• Machine learning analysis of Photometric data from the Dark Energy Survey
• Sustainability of multi-field inflation and bound on string scale
• Constraints on the velocity dispersion of Dark Matter from Cosmology and new bounds on scattering from the Cosmic Dawn
• The Measurement of the Hubble Constant H_0 in the Solar System
• Search for a Dark Matter component
• An Optimal In-Situ Multipole Algorithm for the Isotropic Three-Point Correlation Functions