Cosmology and fundamental physics with the Euclid satellite

Abstract

Euclid is a European Space Agency medium class mission selected for launch in 2019 within the Cosmic Vision 2015-2025 programme. The main goal of Euclid is to understand the origin of the accelerated expansion of the Universe. Euclid will explore the expansion history of the Universe and the evolution of cosmic structures by measuring shapes and redshifts of galaxies as well as the distribution of clusters of galaxies over a large fraction of the sky. Although the main driver for Euclid is the nature of dark energy, Euclid science covers a vast range of topics, from cosmology to galaxy evolution to planetary research. In this review we focus on cosmology and fundamental physics, with a strong emphasis on science beyond the current standard models. We discuss five broad topics: dark energy and modified gravity, dark matter, initial conditions, basic assumptions and questions of methodology in the data analysis. This review has been planned and carried out within Euclid's Theory Working Group and is meant to provide a guide to the scientific themes that will underlie the activity of the group during the preparation of the Euclid mission.

236 pages, minor edits to match the journal version 2013

References in corpus (392)

• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Cosmology and the Fate of Dilatation Symmetry
• A direct empirical proof of the existence of dark matter
• The Standard Model Higgs boson as the inflaton
• Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
• Resummation of Massive Gravity
• Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
• The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey
• Disappearing cosmological constant in f(R) gravity
• Bayes in the sky: Bayesian inference and model selection in cosmology
• The Effective Field Theory of Inflation
• Covariant Galileon
• The Kinematics of the Ultra-Faint Milky Way Satellites: Solving the Missing Satellite Problem
• Observational Signatures and Non-Gaussianities of General Single Field Inflation
• Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds
• Monodromy in the CMB: Gravity Waves and String Inflation
• The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
• Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-5
• Conditions for the cosmological viability of f(R) dark energy models
• A test of the nature of cosmic acceleration using galaxy redshift distortions
• Can dark energy evolve to the Phantom?
• Effective Field Theory for Inflation
• Planck 2013 results. XXIII. Isotropy and statistics of the CMB
• Are f(R) dark energy models cosmologically viable ?
• Starting the Universe: Stable Violation of the Null Energy Condition and Non-standard Cosmologies
• Avoiding Dark Energy with 1/R Modifications of Gravity
• The Large Scale Structure of f(R) Gravity
• The Effective Field Theory of Dark Energy
• On Born-Infeld Gravity in Weitzenbock spacetime
• Inflationary Cosmology
• Bose-Einstein Condensation of Dark Matter Axions
• Light Sterile Neutrinos: A White Paper
• On the Robustness of the Acoustic Scale in the Low-Redshift Clustering of Matter
• Observational signatures of f(R) dark energy models that satisfy cosmological and local gravity constraints
• A Parameterized Post-Friedmann Framework for Modified Gravity
• Measuring the dark side (with weak lensing)
• Essential Building Blocks of Dark Energy
• Large-scale instability in interacting dark energy and dark matter fluids
• Constraining f(R) Gravity as a Scalar Tensor Theory
• Effects of Baryons and Dissipation on the Matter Power Spectrum
• An introduction to the Vainshtein mechanism
• Evading Equivalence Principle Violations, Cosmological and other Experimental Constraints in Scalar Field Theories with a Strong Coupling to Matter
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectra
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). An unprecedented view of galaxies and large-scale structure at 0.5<z<1.2
• Can sterile neutrinos be the dark matter?
• Planck 2013 results. XXV. Searches for cosmic strings and other topological defects
• New Ekpyrotic Cosmology
• New Perspective on Galaxy Clustering as a Cosmological Probe: General Relativistic Effects
• Environmental Dependence of Masses and Coupling Constants
• Vector Inflation
• Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological Implications
• String-inspired Gauss-Bonnet gravity reconstructed from the universe expansion history and yielding the transition from matter dominance to dark energy
• Dark Energy or Modified Gravity? An Effective Field Theory Approach
• f(R) Gravity and Chameleon Theories
• Dynamics of dark energy with a coupling to dark matter
• Distinguishing Modified Gravity from Dark Energy
• Interacting Spin-2 Fields
• Strong and weak lensing united III: Measuring the mass distribution of the merging galaxy cluster 1E0657-56
• Revealing the properties of dark matter in the merging cluster MACSJ0025.4-1222
• Velocity Dispersion Profiles of Seven Dwarf Spheroidal Galaxies
• Hemispherical power asymmetry in the three-year Wilkinson Microwave Anisotropy Probe sky maps
• Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications
• Effects of Scale-Dependent Non-Gaussianity on Cosmological Structures
• Dynamics of interacting dark energy
• The Uncorrelated Universe: Statistical Anisotropy and the Vanishing Angular Correlation Function in WMAP Years 1-3
• Enhanced Non-Gaussianity from Excited Initial States
• Non-Gaussianities in two-field inflation
• Evidence for massive neutrinos from CMB and lensing observations
• Searching for modified growth patterns with tomographic surveys
• Recovering galaxy star formation and metallicity histories from spectra using VESPA
• A general test of the Copernican Principle
• Degravitation of the Cosmological Constant and Graviton Width
• DBI and the Galileon reunited
• Non-linear Evolution of f(R) Cosmologies III: Halo Statistics
• Scale invariance, unimodular gravity and dark energy
• The Effective Theory of Quintessence: the w<-1 Side Unveiled
• The bispectrum of galaxies from high-redshift galaxy surveys: primordial non-Gaussianity and non-linear galaxy bias
• Discreteness effects in simulations of Hot/Warm dark matter
• A Model For Halo Formation With Axion Mixed Dark Matter
• Effective Field Theory of Cosmic Acceleration: an implementation in CAMB
• Dark Matter from new Technicolor Theories
• On the consistency relation of the 3-point function in single field inflation
• $\nu \Lambda$CDM: Neutrinos help reconcile Planck with the Local Universe
• Instability of anisotropic cosmological solutions supported by vector fields
• Testing gravity with CAMB and CosmoMC
• Confronting Lemaitre-Tolman-Bondi models with Observational Cosmology
• Dark Energy versus Modified Gravity
• Thawing quintessence with a nearly flat potential
• Equivalence Principle Implications of Modified Gravity Models
• Neutrinoless double beta decay and neutrino physics
• Colliding clusters and dark matter self-interactions
• The Aspen--Amsterdam Void Finder Comparison Project
• Cosmic Acceleration and the Helicity-0 Graviton
• Non-linear evolution of f(R) cosmologies II: power spectrum
• How cold is cold dark matter? Small scales constraints from the flux power spectrum of the high-redshift Lyman-alpha forest
• N-body Simulations for f(R) Gravity using a Self-adaptive Particle-Mesh Code
• Cosmic Microwave Background Quadrupole and Ellipsoidal Universe
• The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks Versus Substructures
• Current constraints on the cosmic growth history
• The Nature of Primordial Fluctuations from Anisotropic Inflation
• The velocity function in the local environment from LCDM and LWDM constrained simulations
• A Hemispherical Power Asymmetry from Inflation
• Cosmic Microwave Background Statistics for a Direction-Dependent Primordial Power Spectrum
• Realistic sterile neutrino dark matter with keV mass does not contradict cosmological bounds
• Accelerated expansion from ghost-free bigravity: a statistical analysis with improved generality
• Coupled and Extended Quintessence: theoretical differences and structure formation
• Modified Gravity-GADGET: A new code for cosmological hydrodynamical simulations of modified gravity models
• Screening Modifications of Gravity through Disformally Coupled Fields
• Growing Matter
• Semiclassical relations and IR effects in de Sitter and slow-roll space-times
• Lemaitre-Tolman-Bondi model and accelerating expansion
• The universe seen at different scales
• Dark Matter Halo Merger Histories Beyond Cold Dark Matter: I - Methods and Application to Warm Dark Matter
• Ultra-Light Scalar Fields and the Growth of Structure in the Universe
• Non-linear evolution of f(R) cosmologies I: methodology
• The Tensor-Vector-Scalar theory and its cosmology
• The Parameterized Post-Friedmann Framework for Theories of Modified Gravity: Concepts, Formalism and Examples
• Predictions from an anisotropic inflationary era
• Non-Local Modification of Gravity and the Cosmological Constant Problem
• Detection of hot gas in the filament connecting the clusters of galaxies Abell 222 and Abell 223
• Probing String Theory with Modulated Cosmological Fluctuations
• Dark Interactions and Cosmological Fine-Tuning
• Accelerated expansion from structure formation
• Observational constraints on self-accelerating cosmology
• Constraining Interactions in Cosmology's Dark Sector
• Primordial fluctuations and non-Gaussianities in multi-field DBI inflation
• Cosmic variance and the measurement of the local Hubble parameter
• On the growth of linear perturbations
• Constraints on scalar-tensor models of dark energy from observational and local gravity tests
• A Test of the Copernican Principle
• How to optimally parametrize deviations from General Relativity in the evolution of cosmological perturbations
• Cascading DGP
• The Warm DM halo mass function below the cut-off scale
• Signature of the interaction between dark energy and dark matter in galaxy clusters
• Growing neutrinos and cosmological selection
• Cosmological Constraints on f(R) Acceleration Models
• Observables and unobservables in dark energy cosmologies
• Anisotropic Dark Energy: Dynamics of Background and Perturbations
• A practical approach to cosmological perturbations in modified gravity
• Measuring the matter density using baryon oscillations in the SDSS
• Laser experiments explore the hidden sector
• The Effect of Thermal Neutrino Motion on the Non-linear Cosmological Matter Power Spectrum
• Polarized Light Propagating in a Magnetic Field as a Probe of Millicharged Fermions
• On model selection forecasting, Dark Energy and modified gravity
• Can a vector field be responsible for the curvature perturbation in the Universe?
• Probing modifications of General Relativity using current cosmological observations
• CMB anisotropies seen by an off-center observer in a spherically symmetric inhomogeneous universe
• Einstein and Jordan frames reconciled: a frame-invariant approach to scalar-tensor cosmology
• CFHTLenS: Mapping the Large Scale Structure with Gravitational Lensing
• Non-Gaussianities in New Ekpyrotic Cosmology
• Impact of massive neutrinos on nonlinear matter power spectrum
• Can Cosmic Structure form without Dark Matter?
• Constraints on a New Post-General Relativity Cosmological Parameter
• Matter density perturbations in interacting quintessence models
• Quasi-Dilaton: Theory and Cosmology
• Cosmology with massive neutrinos III: the halo mass function and an application to galaxy clusters
• Illuminating the Hidden Sector of String Theory by Shining Light through a Magnetic Field
• The nonlinear matter and velocity power spectra in f(R) gravity
• A filament of dark matter between two clusters of galaxies
• Effect of baryonic feedback on two- and three-point shear statistics: prospects for detection and improved modelling
• Phantom dark energy from non-local infrared modifications of General Relativity
• Planck 2013 results. XXVI. Background geometry and topology of the Universe
• The Growth of Structure in Interacting Dark Energy Models
• Efficient Bayesian inference for multimodal problems in cosmology
• How to suppress the shot noise in galaxy surveys
• Dark Matter Candidates - Axions, Neutralinos, Gravitinos, and Axinos
• Cosmic Degeneracies I: Joint N-body Simulations of Modified Gravity and Massive Neutrinos
• Isocurvature bounds on axions revisited
• Figure of Merit for Dark Energy Constraints from Current Observational Data
• A Weak-Lensing Mass Reconstruction of the Large-Scale Filament Feeding the Massive Galaxy Cluster MACSJ0717.5+3745
• ISIS: a new N-body cosmological code with scalar fields based on RAMSES. Code presentation and application to the shapes of clusters
• Redshift space distortions in f(R) gravity
• Improved Primordial Non-Gaussianity Constraints from Measurements of Galaxy Clustering and the Integrated Sachs-Wolfe Effect
• Non-Renormalization and Naturalness in a Class of Scalar-Tensor Theories
• Density perturbations in general modified gravitational theories
• Non-Gaussian Spikes from Chaotic Billiards in Inflation Preheating
• Density perturbations in f(R) gravity theories in metric and Palatini formalisms
• Crossing the Phantom Divide
• A new life for sterile neutrinos: resolving inconsistencies using hot dark matter
• Constraining Dark Energy Anisotropic Stress
• Looking the void in the eyes - the kSZ effect in LTB models
• Axions as Quintessence in String Theory
• A Bayesian model selection analysis of WMAP3
• Hilltop Quintessence
• Coupled dark matter-dark energy in light of near Universe observations
• Differentiating dark energy and modified gravity with galaxy redshift surveys
• On the formation of dwarf galaxies and stellar halos
• Releasing scalar fields: cosmological simulations of scalar-tensor theories for gravity beyond the static approximation
• Anisotropic Friedmann-Robertson-Walker universe from nonlinear massive gravity
• Constraining Isocurvature Initial Conditions with WMAP 3-year data
• Beyond the plane-parallel and Newtonian approach: Wide-angle redshift distortions and convergence in general relativity
• Observational constraints on the linear fluctuation growth rate
• Testing the Void against Cosmological data: fitting CMB, BAO, SN and H0
• No-go theorem for k-essence dark energy
• Interacting models of soft coincidence
• On the Stability of a class of Modified Gravitational Models
• Asymmetric Beams and CMB Statistical Anisotropy
• Non-Gaussianities from ekpyrotic collapse with multiple fields
• Exploring Vainshtein mechanism on adaptively refined meshes
• Scalar Perturbations on Lemaitre-Tolman-Bondi Spacetimes
• Precision cosmology defeats void models for acceleration
• Quantum Corrections in Massive Gravity
• Nonlinear power spectrum in the presence of massive neutrinos: perturbation theory approach, galaxy bias and parameter forecasts
• How early is early dark energy?
• N-Body Simulations of DGP and Degravitation Theories
• Constraints on cosmic hemispherical power anomalies from quasars
• The significance of the integrated Sachs-Wolfe effect revisited
• The bispectrum of redshifted 21-cm fluctuations from the dark ages
• GaBoDS: The Garching-Bonn Deep Survey -- IX. A sample of 158 shear-selected mass concentration candidates
• Comparing Infrared Dirac-Born-Infeld Brane Inflation to Observations
• Lensing, reddening and extinction effects of MgII absorbers from z=0.4 to z=2
• Present and future evidence for evolving dark energy
• Constraints on dark matter particles from theory, galaxy observations and N-body simulations
• The dark matter environment of the Abell 901/902 supercluster: a weak lensing analysis of the HST STAGES survey
• Accurate estimators of power spectra in N-body simulations
• Signature of Primordial Non-Gaussianity on Matter Power Spectrum
• Detecting a Lorentz-Violating Field in Cosmology
• The CMB cold spot: texture, cluster or void?
• The Cosmology of Ricci-Tensor-Squared Gravity in the Palatini Variational Approach
• Observational signatures of Jordan-Brans-Dicke theories of gravity
• Simulating the quartic Galileon gravity model on adaptively refined meshes
• Vector field models of modified gravity and the dark sector
• Finding Evidence for Massive Neutrinos using 3D Weak Lensing
• Neutrino Dark Energy -- Revisiting the Stability Issue
• Findings of the Joint Dark Energy Mission Figure of Merit Science Working Group
• General Relativistic N-body simulations in the weak field limit
• Effects and Detectability of Quasi-Single Field Inflation in the Large-Scale Structure and Cosmic Microwave Background
• On the onset of cosmological backreaction
• A Scale-Dependent Power Asymmetry from Isocurvature Perturbations
• Recovering 3D clustering information with angular correlations
• Dark Coupling and Gauge Invariance
• Neutrino clustering in growing neutrino quintessence
• The Three-Point Correlation Function of Luminous Red Galaxies in the Sloan Digital Sky Survey
• Weak lensing survey of galaxy clusters in the CFHTLS Deep
• Fingerprinting dark energy
• 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
• Unified Dark Matter Scalar Field Models
• Anisotropic non-Gaussianity from vector field perturbations
• Consistency among distance measurements: transparency, BAO scale and accelerated expansion
• Hunting Down the Best Model of Inflation with Bayesian Evidence
• Testable polarization predictions for models of CMB isotropy anomalies
• Sterile Neutrinos in Light of Recent Cosmological and Oscillation Data: a Multi-Flavor Scheme Approach
• Scattering of Dark Matter and Dark Energy
• Cosmological constraints from COMBO-17 using 3D weak lensing
• Cosmological simulations of screened modified gravity out of the static approximation: effects on matter distribution
• New constraints on Parity Symmetry from a re-analysis of the WMAP-7 low resolution power spectra
• On the growth of structure in theories with a dynamical preferred frame
• Phantom boundary crossing and anomalous growth index of fluctuations in viable f(R) models of cosmic acceleration
• Eddington-Born-Infeld gravity and the large scale structure of the Universe
• $\Lambda \alpha$DM: Observational constraints on unified dark matter with constant speed of sound
• SPACE: the SPectroscopic All-sky Cosmic Explorer
• The Void Abundance with Non-Gaussian Primordial Perturbations
• Spherical collapse and halo mass function in f(R) theories
• Testing the Copernican principle by constraining spatial homogeneity
• Slow-roll k-essence
• Cosmological Parameter Estimation with Large Scale Structure Observations
• Clarifying spherical collapse in coupled dark energy cosmologies
• Seeing patterns in noise: Gigaparsec-scale `structures' that do not violate homogeneity
• The radial BAO scale and Cosmic Shear, a new observable for Inhomogeneous Cosmologies
• Mass functions in coupled Dark Energy models
• Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• Constraining Primordial Non-Gaussianity with High-Redshift Probes
• CMB Lensing Constraints on Neutrinos and Dark Energy
• Chameleon dark energy models with characteristic signatures
• A Covariant Master Theory for Novel Galilean Invariant Models and Massive Gravity
• The Odd-Parity CMB Bispectrum
• Direction-Dependent CMB Power Spectrum and Statistical Anisotropy from Noncommutative Geometry
• Confronting General Relativity with Further Cosmological Data
• Cosmological Evolution of Interacting Dark Energy Models with Mass Varying Neutrinos
• Non-minimally coupled vector curvaton
• Linear kinetic Sunyaev-Zel'dovich effect and void models for acceleration
• Weak lensing study of dark matter filaments and application to the binary cluster A 222 and A 223
• The Impact of Cosmic Dust on Supernova Cosmology
• A sub-horizon framework for probing the relationship between the cosmological matter distribution and metric perturbations
• Neutrino Mass, Dark Energy, and the Linear Growth Factor
• The cosmological behavior of Bekenstein's modified theory of gravity
• New interactions in the dark sector mediated by dark energy
• Forecasting the Bayes factor of a future observation
• Triple unification of inflation, dark matter, and dark energy using a single field
• Using correlations between CMB lensing and large-scale structure to measure primordial non-Gaussianity
• Microscopic and Macroscopic Behaviors of Palatini Modified Gravity Theories
• Magnetic Mixing -- Electric Minicharges from Magnetic Monopoles
• Supernova Brightening from Chameleon-Photon Mixing
• The linear growth rate of structure in Parametrized Post Friedmannian Universes
• The latitude dependence of the rotation measures of NVSS sources
• Cosmology of the selfaccelerating third order Galileon
• Combining Planck with Large Scale Structure gives strong neutrino mass constraint
• Anisotropic perturbations due to dark energy
• Neutrino mass constraint with the Sloan Digital Sky Survey power spectrum of luminous red galaxies and perturbation theory
• Cosmologies of extended massive gravity
• Measuring deviations from a cosmological constant: a field-space parameterization
• Topology and Dark Energy: Testing Gravity in Voids
• Non-detection of a statistically anisotropic power spectrum in large-scale structure
• Ekpyrotic Perturbations With Small Non-Gaussian Corrections
• Dark Energy as a Modification of the Friedmann Equation
• The Integrated Sachs-Wolfe effect in $f(R)$ gravity
• Coupled three-form dark energy
• Late universe dynamics with scale-independent linear couplings in the dark sector
• On Adiabatic Renormalization of Inflationary Perturbations
• Future CMB cosmological constraints in a dark coupled universe
• A Complete Statistical Analysis for the Quadrupole Amplitude in an Ellipsoidal Universe
• Probing Dark Energy through Scale Dependence
• Cosmic Parallax: possibility of detecting anisotropic expansion of the universe by very accurate astrometry measurements
• Accurate weak lensing of standard candles. I. Flexible cosmological fits
• Cosmological Systematics Beyond Nuisance Parameters : Form Filling Functions
• Current Status Of Velocity Field Surveys: A Consistency Check
• Constraining warm dark matter with cosmic shear power spectra
• Testing Cosmology with Cosmic Sound Waves
• Constraining Modified Gravity with Euclid
• Examples of backreaction of small scale inhomogeneities in cosmology
• Planck priors for dark energy surveys
• Cosmology with the Square Kilometre Array
• On the cross-section of Dark Matter using substructure infall into galaxy clusters
• Probing deviations from General Relativity with the Euclid spectroscopic survey
• A new method for the Alcock-Paczynski test
• Detectability of Torsion Gravity via Galaxy Clustering and Cosmic Shear Measurements
• Accurate Weak Lensing of Standard Candles. II. Measuring sigma8 with Supernovae
• Future weak lensing constraints in a dark coupled universe
• Speed of Sound in the Mass Varying Neutrinos Scenario
• Power Asymmetries in the Cosmic Microwave Background Temperature and Polarization patterns
• Toward a Unified Description of Dark Energy and Dark Matter from the Abnormally Weighting Energy Hypothesis
• Radial density profiles of time-delay lensing galaxies
• The Redshift Sensitivities of Dark Energy Surveys
• A Coverage Study of the CMSSM Based on ATLAS Sensitivity Using Fast Neural Networks Techniques
• Cold Dark Matter Isocurvature Perturbations: Constraints and Model Selection
• Fingerprinting Dark Energy II: weak lensing and galaxy clustering tests
• Anisotropic stress and stability in modified gravity models
• Naturalness of exponential cosmon potentials and the cosmological constant problem
• Dark Energy coupling with electromagnetism as seen from future low-medium redshift probes
• Probing Dark Energy at Galactic and Cluster Scales
• Internal Robustness: systematic search for systematic bias in SN Ia data
• Neutrino lumps and the Cosmic Microwave Background
• Lyman-α Forest and Cosmic Weak Lensing in a Warm Dark Matter Universe
• Optimising Baryon Acoustic Oscillation Surveys - I: Testing the concordance LCDM cosmology
• Can F(R)-gravity be a viable model: the universal unification scenario for inflation, dark energy and dark matter
• Two strong-lensing clusters confront universal dark-matter profiles
• LTB universes as alternatives to dark energy: does positive averaged acceleration imply positive cosmic acceleration?
• Unified model of baryonic matter and dark components
• Deconstructing Baryon Acoustic Oscillations: A Comparison of Methods
• Model selection forecasts for the spectral index from the Planck satellite
• Varying couplings in the early universe: correlated variations of $\alpha$ and $G$
• Uncertainty on w from large-scale structure
• Dark Matter Structures In The Deep Lens Survey
• CMB statistics in noncommutative inflation
• Unification of inflation, dark energy, and dark matter within the Salam-Sezgin cosmological model
• DEUS Full Observable ΛCDM Universe Simulation: the numerical challenge
• Isocurvature modes and Baryon Acoustic Oscillations
• The Hubble diagram as a probe of mini-charged particles
• Neutrino Lumps in Quintessence Cosmology
• Unifying cosmological and recent time variations of fundamental couplings
• Characterizing dark interactions with the halo mass accretion history and structural properties
• An Improved Semi-Analytical Spherical Collapse Model for Non-linear Density Evolution
• Quantum backreaction in evolving FLRW spacetimes
• Non-linear weak lensing forecasts
• Structure formation in Multiple Dark Matter cosmologies with long-range scalar interactions
• The cluster lens ACO 1703: redshift contrast and the inner profile
• Measuring the transition to homogeneity with photometric redshift surveys
• The Cold Spot as a Large Void: Rees-Sciama effect on CMB Power Spectrum and Bispectrum
• Studying Inter-Cluster Galaxy Filaments Through Stacking GMBCG Galaxy Cluster Pairs
• Anisotropies in the Cosmic Neutrino Background after WMAP 5-year Data
• Route to Lambda in conformally coupled phantom cosmology
• Should we doubt the cosmological constant?
• Intrinsic uncertainty on the nature of dark energy
• Parameterizing and Measuring Dark Energy Trajectories from Late-Inflatons
• Indistinguishable Macroscopic Behaviour of Palatini Gravities and General Relativity
• Covariant Linear Perturbation Formalism
• Dark Matter Astrometry: Accuracy of sub-halo positions for the measurement of self-interaction cross sections
• When can the Planck satellite measure spectral index running?
• Application of Bayesian model averaging to measurements of the primordial power spectrum
• Hydrodynamical simulations of coupled and uncoupled quintessence models II: Galaxy clusters
• Cosmology of Chameleons with Power-Law Couplings
• Constraining TeVeS Gravity as Effective Dark Matter and Dark Energy
• Dark Matter, Modified Gravity and the Mass of the Neutrino
• Cusp-core problem and strong gravitational lensing
• Weak lensing detection of intra-cluster filaments with ground based data
• A Multi-Resolution Weak Lensing Mass Reconstruction Method
• Galaxy clusters and the cosmic cycle of baryons across cosmic times
• Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys
• Halo abundances and shear in void models
• CMB anisotropies from acausal scaling seeds
• The dark aftermath of Higgs inflation
• Structure and evolution of Zel'dovich pancakes as probes of dark energy models
• Phantom behaviour and growth index anomalous evolution in viable f(R) gravity models
• Constraints on the decay of dark matter to dark energy from weak lensing bispectrum tomography
• eROSITA on SRG: a X-ray all-sky survey mission
• Dark matter halo formation in the multicomponent dark matter models
• Dark Energy Phenomenology
• Astrophysics and cosmology with galaxy clusters: the WFXT perspective
• Triple Unification of Inflation, Dark matter and Dark energy in Chaotic Braneworld Inflation
• Growing neutrino cosmology

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• Measuring Dark Energy Properties with Photometrically Classified Pan-STARRS Supernovae. II. Cosmological Parameters
• Neutrino masses and cosmological parameters from a Euclid-like survey: Markov Chain Monte Carlo forecasts including theoretical errors
• gevolution: a cosmological N-body code based on General Relativity
• Modified Gravity N-body Code Comparison Project
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• Phantom dark energy from non-local infrared modifications of General Relativity
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• 3D Cosmic Shear: Cosmology from CFHTLenS
• The fate of large-scale structure in modified gravity after GW170817 and GRB170817A
• The promising future of a robust cosmological neutrino mass measurement
• Primordial non-gaussianity from the bispectrum of 21-cm fluctuations in the dark ages
• Hunting down horizon-scale effects with multi-wavelength surveys
• Effects of nonlinear inhomogeneity on the cosmic expansion with numerical relativity
• Scalar-tensor theories of gravity, neutrino physics, and the $H_0$ tension
• Effective Theory of Interacting Dark Energy
• A Compendium of Chameleon Constraints
• Galaxy Power Spectrum Multipoles Covariance in Perturbation Theory
• Defining a weak lensing experiment in space
• Modelling the number density of Halpha emitters for future spectroscopic near-IR space missions
• Cosmological perturbation theory at three-loop order
• Are peculiar velocity surveys competitive as a cosmological probe?
• Galaxy number counts to second order and their bispectrum
• Barrow holographic dark energy with Hubble horizon as IR cutoff
• Cosmological Constraints From Weak Lensing Peak Statistics With CFHT Stripe 82 Survey
• Cosmographic Constraints and Cosmic Fluids
• Negative cosmological constant in the dark sector?
• Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
• The Euclid mission design
• Cosmological Applications of Pade Approximant
• Estimating Cosmological Parameter Covariance
• Interpreting measurements of the anisotropic galaxy power spectrum
• Extending cosmological tests of General Relativity with the Square Kilometre Array
• Cosmology in the era of Euclid and the Square Kilometre Array
• Internal Robustness of Growth Rate data
• AX-GADGET: a new code for cosmological simulations of Fuzzy Dark Matter and Axion models
• Cosmological performance of SKA HI galaxy surveys
• Constraining $f(R)$ Gravity Theory Using Weak Lensing Peak Statistics from the Canada-France-Hawaii-Telescope Lensing Survey
• Looking through the same lens: shear calibration for LSST, Euclid & WFIRST with stage 4 CMB lensing
• Relaxing Cosmological Neutrino Mass Bounds with Unstable Neutrinos
• A study of the sensitivity of shape measurements to the input parameters of weak lensing image simulations
• Observational constraints on generalized Proca theories
• Non-Gaussian Covariance of the Matter Power Spectrum in the Effective Field Theory of Large Scale Structure
• Einstein's legacy in galaxy surveys
• Effective Theory of Dark Energy at Redshift Survey Scales
• Fast and accurate mock catalogue generation for low-mass galaxies
• Cosmological Measurements with General Relativistic Galaxy Correlations
• Probing primordial features with future galaxy surveys
• Structure formation in inhomogeneous Early Dark Energy models
• The Abell 3391/95 galaxy cluster system: A 15 Mpc intergalactic medium emission filament, a warm gas bridge, infalling matter clumps, and (re-) accelerated plasma discovered by combining SRG/eROSITA data with ASKAP/EMU and DECam data
• $Euclid$ preparation: XV. Forecasting cosmological constraints for the $Euclid$ and CMB joint analysis
• Structure formation with massive neutrinos: going beyond linear theory
• Hidden Negative Energies in Strongly Accelerated Universes
• On the Role of $f(G,T)$ Terms in Structure Scalars
• The BOSS bispectrum analysis at one loop from the Effective Field Theory of Large-Scale Structure
• Direct detection of gravitational waves can measure the time variation of the Planck mass
• The power spectrum and bispectrum of SDSS DR11 BOSS galaxies II: cosmological interpretation
• Tension of the $E_G$ statistic and RSD data with Planck/$\Lambda$CDM and implications for weakening gravity
• Bias due to neutrinos must not uncorrect'd go
• Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure
• Relativistic N-body simulations with massive neutrinos
• On the road to percent accuracy IV: ReACT -- computing the non-linear power spectrum beyond $\Lambda$CDM
• Tests of Gravity with Future Space-Based Experiments
• High-redshift post-reionization cosmology with 21cm intensity mapping
• Breaking of the equivalence principle in the electromagnetic sector and its cosmological signatures
• Measuring the lensing potential with tomographic galaxy number counts
• K-mouflage Cosmology: the Background Evolution
• Constraining $f(R)$ gravity by the Large Scale Structure
• Breaking the spell of Gaussianity: forecasting with higher order Fisher matrices
• Quintessence Saves Higgs Instability
• Nonlinear structure formation in Nonlocal Gravity
• More out of less: an excess integrated Sachs-Wolfe signal from supervoids mapped out by the Dark Energy Survey
• On the linearity of tracer bias around voids
• Measurement of the $T_{\mathrm{CMB}}$ evolution from the Sunyaev-Zel'dovich effect
• The Future of Primordial Features with Large-Scale Structure Surveys
• Accurate cosmic shear errors: do we need ensembles of simulations?
• CMB weak-lensing beyond the Born approximation: a numerical approach
• The full-sky relativistic correlation function and power spectrum of galaxy number counts: I. Theoretical aspects
• SKA Weak Lensing I: Cosmological Forecasts and the Power of Radio-Optical Cross-Correlations
• Addressing $H_0$ tension by means of VCDM
• Cosmic voids in coupled dark energy cosmologies: the impact of halo bias
• N-body methods for relativistic cosmology
• Cosmological dynamics and dark energy from non-local infrared modifications of gravity
• The bispectrum of relativistic galaxy number counts
• Cosmology with intensity mapping techniques using atomic and molecular lines
• Cosmology with the Large Synoptic Survey Telescope: an Overview
• Verifying the consistency relation for the scale-dependent bias from local primordial non-Gaussianity
• A novel approach in the WIMP quest: Cross-Correlation of Gamma-Ray Anisotropies and Cosmic Shear
• Model-independent constraints on the cosmological anisotropic stress
• Modeling Galaxies in Redshift Space at the Field Level
• Stellar Oscillations in Modified Gravity
• Encyclopaedia Curvatonis
• Probing Cosmological Isotropy With Type IA Supernovae
• Cosmological constraints on induced gravity dark energy models
• Nonlinear Effective Theory of Dark Energy
• Constraining power of asymptotic safety for scalar fields
• Exploring cosmic origins with CORE: gravitational lensing of the CMB
• A comparison of structure formation in minimally and non-minimally coupled quintessence models
• Linear growth of structure in massive bigravity
• Cosmology in bimetric theory with an effective composite coupling to matter
• Constraints on interacting dark energy models through cosmic chronometers and Gaussian process
• Dark Energy and Modified Gravity in the Effective Field Theory of Large-Scale Structure
• Exploiting the full potential of photometric quasar surveys: Optimal power spectra through blind mitigation of systematics
• Phenomenology of theories of gravity without Lorentz invariance: the preferred frame case
• Cosmic Shear Covariance Matrix in $w$CDM: Cosmology Matters
• DEMNUni: Massive neutrinos and the bispectrum of large scale structures
• Cosmological neutrino simulations at extreme scale
• Changing the prior: absolute neutrino mass constraints in nonlocal gravity
• Star-galaxy separation strategies for WISE-2MASS all-sky infrared galaxy catalogs
• CMB lensing reconstruction biases in cross-correlation with large-scale structure probes
• Testing AdS early dark energy with Planck, SPTpol and LSS data
• Shaken, not stirred: kinetic mixing in scalar-tensor theories of gravity
• Probing reheating with primordial spectrum
• A general theory of linear cosmological perturbations: scalar-tensor and vector-tensor theories
• Large-scale 3D galaxy correlation function and non-Gaussianity
• A Realistic U(2) Model of Flavor
• Anisotropies of gravitational-wave standard sirens as a new cosmological probe without redshift information
• Moduli Vacuum Misalignment and Precise Predictions in String Inflation
• Health checkup test of the standard cosmological model in view of recent Cosmic Microwave Background Anisotropies experiments
• ${\varphi }^2$ or Not ${\varphi }^2$: Testing the Simplest Inflationary Potential
• Extending the supernova Hubble diagram to z~1.5 with the Euclid space mission
• Understanding the suppression of structure formation from dark matter$\unicode{x2013}$dark energy momentum coupling
• Analytic study of the effect of dark energy-dark matter interaction on the growth of structures
• Matter Power Spectrum Covariance Matrix from the DEUS-PUR ΛCDM simulations: Mass Resolution and non-Gaussian Errors
• Topology and Dark Energy: Testing Gravity in Voids
• K-mouflage Cosmology: Formation of Large-Scale Structures
• The missing link: a nonlinear post-Friedmann framework for small and large scales
• Distinguishing interacting dark energy from wCDM with CMB, lensing, and baryon acoustic oscillation data
• Dark matter and halo bispectrum in redshift space: theory and applications
• Determining the Neutrino Lifetime from Cosmology
• Biases from neutrino bias: to worry or not to worry?
• Mirror Twin Higgs Cosmology: Constraints and a Possible Resolution to the $H_0$ and $S_8$ Tensions
• Cosmological Signatures of Superheavy Dark Matter
• Higgs-Dilaton Cosmology: An inflation - dark energy connection and forecasts for future galaxy surveys
• Non-local gravity and comparison with observational datasets. II. Updated results and Bayesian model comparison with $\Lambda$CDM
• Unveiling the Dynamics of the Universe
• Primordial Gravitational Waves from Galaxy Intrinsic Alignments
• The 400d Galaxy Cluster Survey weak lensing programme: III: Evidence for consistent WL and X-ray masses at $z\approx 0.5$
• Euclid Mission: building of a Reference Survey
• Inferring $S_8(z)$ and $\gamma (z)$ with cosmic growth rate measurements using machine learning
• Testing (modified) gravity with 3D and tomographic cosmic shear
• Supervoids in the WISE-2MASS catalogue imprinting Cold Spots in the Cosmic Microwave Background
• An improved measurement of baryon acoustic oscillations from the correlation function of galaxy clusters at $z\sim 0.3$
• The Atacama Cosmology Telescope: measuring radio galaxy bias through cross-correlation with lensing
• Cosmological constraints on deviations from Lorentz invariance in gravity and dark matter
• A general theory of linear cosmological perturbations: stability conditions, the quasistatic limit and dynamics
• Sub-millimeter Spatial Oscillations of Newton's Constant: Theoretical Models and Laboratory Tests
• Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
• Tomographic-spectral approach for dark matter detection in the cross-correlation between cosmic shear and diffuse gamma-ray emission
• Observational signatures of modified gravity on ultra-large scales
• Modified gravity for surveys
• On the importance of lensing for galaxy clustering in photometric and spectroscopic surveys
• The Hunt for Primordial Interactions in the Large Scale Structures of the Universe
• The Cosmic Microwave Background: The history of its experimental investigation and its significance for cosmology
• Cosmology with dropout selection: Straw-man surveys and CMB lensing
• Lensing convergence and the neutrino mass scale in galaxy redshift surveys
• Gravity in the infrared and effective nonlocal models
• Cosmic variance limited Baryon Acoustic Oscillations from the DEUS-FUR $\Lambda$CDM simulation
• Axionic black branes in the k-essence sector of the Horndeski model
• Constraining interacting dark energy with CMB and BAO future surveys
• Principal Component Analysis of Modified Gravity using Weak Lensing and Peculiar Velocity Measurements
• Scaling solutions and weak gravity in dark energy with energy and momentum couplings
• Optimising growth of structure constraints on modified gravity
• Cosmological constraints from a joint analysis of cosmic growth and expansion
• Solar System Constraints on Disformal Gravity Theories
• New constraints on ${\sigma }_8$ from a joint analysis of stacked gravitational lensing and clustering of galaxy clusters
• Large-scale redshift space distortions in modified gravity theories
• Weakening Gravity on Redshift-Survey Scales with Kinetic Matter Mixing
• Variable sound speed in interacting dark energy models
• Double shadows of reflection-asymmetric wormholes supported by positive energy thin-shells
• Limits on primordial non-Gaussianities from BOSS galaxy-clustering data
• Hints of dark matter-neutrino interactions in Lyman-$\alpha$ data
• How to relax the cosmological neutrino mass bound
• A Hybrid Deep Learning Approach to Cosmological Constraints From Galaxy Redshift Surveys
• Robust Field-level Likelihood-free Inference with Galaxies
• Safely smoothing spacetime: backreaction in relativistic cosmological simulations
• Reconstructing Horndeski theories from phenomenological modified gravity and dark energy models on cosmological scales
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• A Consistency Relation for the Observed Galaxy Bispectrum and the Local non-Gaussianity from Relativistic Corrections
• Learning effective physical laws for generating cosmological hydrodynamics with Lagrangian Deep Learning
• Cosmological Constraint Precision of the Photometric and Spectroscopic Multi-probe Surveys of China Space Station Telescope (CSST)
• A new approach to the propagation of light-like signals in perturbed cosmological backgrounds
• Future cosmological sensitivity for hot dark matter axions
• Effective Field Theory of Dark Energy: a Dynamical Analysis
• Cosmological distance indicators
• Detectability of Torsion Gravity via Galaxy Clustering and Cosmic Shear Measurements
• GAz: A Genetic Algorithm for Photometric Redshift Estimation
• Clustering-based redshift estimation: application to VIPERS/CFHTLS
• Probing primordial non-Gaussianity via iSW measurements with SKA continuum surveys
• Non-linear evolution of the BAO scale in alternative theories of gravity
• Hiding neutrino mass in modified gravity cosmologies
• Parametrizing modified gravity for cosmological surveys
• An estimation of the Local growth rate from Cosmicflows-3 peculiar velocities
• Imaging Systematics and Clustering of DESI Main Targets
• Probing gravity at large scales through CMB lensing
• Cosmology in scalar-vector-tensor theories
• Quantifying the global "CMB tension" between the Atacama Cosmology Telescope and the Planck satellite in extended models of cosmology
• Galaxy Cluster Mass Reconstruction Project: III. The impact of dynamical substructure on cluster mass estimates
• Halo velocity profiles in screened modified gravity theories
• BAM: Bias Assignment Method to generate mock catalogs
• Prospects for clustering and lensing measurements with forthcoming intensity mapping and optical surveys
• Principal reconstructed modes of dark energy and gravity
• SKA Weak Lensing III: Added Value of Multi-Wavelength Synergies for the Mitigation of Systematics
• Improved constraint on the primordial gravitational-wave density using recent cosmological data and its impact on cosmic string models
• Cosmic homogeneity: a spectroscopic and model-independent measurement
• Isotropy of low redshift type Ia Supernovae: A Bayesian analysis
• Cosmological test of gravity using weak lensing voids
• Measuring the scale of cosmic homogeneity with SDSS-IV DR14 quasars
• Measuring the speed of light with Baryon Acoustic Oscillations
• Measuring gravity at cosmological scales
• Hunting high and low: Disentangling primordial and late-time non-Gaussianity with cosmic densities in spheres
• Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars
• Quintessence in a quandary: prior dependence in dark energy models
• Updating non-standard neutrinos properties with Planck-CMB data and full-shape analysis of BOSS and eBOSS galaxies
• Constraints on the Reheating Parameters after Gauss-Bonnet Inflation from the Primordial Gravitational Waves
• Cosmic inflation in a landscape of heavy-fields
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• Parameterizing dark sector perturbations via equations of state
• Lyman-α Forest and Cosmic Weak Lensing in a Warm Dark Matter Universe
• Dark Energy Survey Year 1 Results: the lensing imprint of cosmic voids on the Cosmic Microwave Background
• Spatial curvature endgame: Reaching the limit of curvature determination
• Optimised angular power spectra for spectroscopic galaxy surveys
• Measuring the distance-redshift relation with the baryon acoustic oscillations of galaxy clusters
• Perturbative description of bias tracers using consistency relations of LSS
• Constraining the general reheating phase in the $\alpha$-attractor inflationary cosmology
• Precision Tests of CO and [CII] Power Spectra Models against Simulated Intensity Maps
• Accuracy of the growth index in the presence of dark energy perturbations
• Toward a concordance teleparallel Cosmology I: Background Dynamics
• Reconstructing Horndeski models from the effective field theory of dark energy
• CosmoBit: A GAMBIT module for computing cosmological observables and likelihoods
• Phantom singularities and their quantum fate: general relativity and beyond
• Weighing Neutrinos in $f(R)$ gravity
• Machine Learning for Observational Cosmology
• Two phase reheating: CMB constraints on inflaton and dark matter phenomenology
• Casimir, Gravitational and Neutron Tests of Dark Energy
• A Measurement of the Cosmic Optical Background and Diffuse Galactic Light Scaling from the R < 50 AU New Horizons-LORRI Data
• Primordial non-Gaussianities and zero bias tracers of the Large Scale Structure
• Optimising primordial non-Gaussianity measurements from galaxy surveys
• Non-standard gravitational waves imply gravitational slip: on the difficulty of partially hiding new gravitational degrees of freedom
• Cosmology with Superluminous Supernovae
• Semi-analytic galaxy formation in f(R)-gravity cosmologies
• Intrinsic alignment contamination to CMB lensing-galaxy weak lensing correlations from tidal torquing
• Synergies between intensity maps of hydrogen lines
• Hairy black hole solutions in $U(1)$ gauge-invariant scalar-vector-tensor theories
• Tomographic Intensity Mapping versus Galaxy Surveys: Observing the Universe in H-alpha emission with new generation instruments
• Cosmic voids detection without density measurements
• Fast and easy super-sample covariance of large scale structure observables
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• Testing the Cosmic Anisotropy with Supernovae Data: Hemisphere Comparison and Dipole Fitting
• Dark energy as a fixed point of the Einstein Yang-Mills Higgs Equations
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): ${\Omega }_{{\mathrm{m}}_0}$ from the galaxy clustering ratio measured at $z\sim 1$
• Principal Shapes and Squeezed Limits in the Effective Field Theory of Large Scale Structure
• A model-independent reconstruction of dark sector interactions
• Strongly Coupled Dark Energy Cosmologies: preserving LCDM success and easing low scale problems II - Cosmological simulations
• Non-linear contributions to angular power spectra
• Evidence for cosmic acceleration with next-generation surveys: A model-independent approach
• Disconnected Covariance of 2-point Functions in Large-Scale Structure
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): Reconstruction of the redshift-space galaxy density field
• Perturbation theory challenge for cosmological parameters estimation: Matter power spectrum in real space
• Pan-STARRS1 variability of XMM-COSMOS AGN. I. Impact on photometric redshifts
• Fundamental cosmology in the E-ELT era: The status and future role of tests of fundamental coupling stability
• Inflationary Constraints on Late Time Modulus Dominated Cosmology
• Higgs Dark Energy
• The sparkling Universe: the coherent motions of cosmic voids
• ProFuse: Physical Multi-Band Structural Decomposition of Galaxies and the Mass-Size-Age Plane
• Radiative Screening of Fifth Forces
• Recovering lost 21 cm radial modes via cosmic tidal reconstruction
• Dark matter haloes in modified gravity and dark energy: interaction rate, small-, and large-scale alignment
• Reheating predictions in Gravity Theories with Derivative Coupling
• Universality for quintessence
• LHC Signatures Of Scalar Dark Energy
• Increasing the Lensing Figure of Merit through Higher Order Convergence Moments
• Horndeski in the Swampland
• Cosmological perturbation theory in Generalized Einstein-Aether models
• Nonlinear evolution of initially biased tracers in modified gravity
• Euclid space mission: a cosmological challenge for the next 15 years
• Gravitational Lens Recovery with GLASS: Measuring the mass profile and shape of a lens
• Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- I. The importance of redshift-space distortions for galaxy number counts
• Non-minimal Derivative Coupling Scalar Field and Bulk Viscous Dark Energy
• Reconciling Planck cluster counts and cosmology? Chandra/XMM instrumental calibration and hydrostatic mass bias
• Towards a non-Gaussian model of redshift space distortions
• Constraining power of cosmological observables: blind redshift spots and optimal ranges
• Low-redshift estimates of the absolute scale of baryon acoustic oscillations
• Detecting Black-Hole Binary Clustering via the Second-Generation Gravitational-Wave Detectors
• Approximation of the potential in scalar field dark energy models
• When is the growth index constant?
• Measuring a Charge-Coupled Device Point Spread Function: Euclid Visible Instrument CCD273-84 PSF Performance
• Euclid preparation III. Galaxy cluster detection in the wide photometric survey, performance and algorithm selection
• Multiple Lensing of the Cosmic Microwave Background anisotropies
• The Halo Void (Dust) Model of Large Scale Structure
• Breaking the Vainshtein screening in clusters of galaxies
• EFTofLSS meets simulation-based inference: ${\sigma }_8$ from biased tracers
• Efficient optimal non-Gaussian CMB estimators with polarisation
• Surfing gravitational waves: can bigravity survive growing tensor modes?
• Computing model independent perturbations in dark energy and modified gravity
• Structure formation in Multiple Dark Matter cosmologies with long-range scalar interactions
• Non-linear general relativistic effects in the observed redshift
• Simulating cosmologies beyond $\Lambda$CDM with PINOCCHIO
• Can Chern-Simons or Rarita-Schwinger be a Volkov-Akulov Goldstone?
• A direct measure of free electron gas via the Kinematic Sunyaev-Zel'dovich effect in Fourier-space analysis
• Cosmological Constant, Fine Structure Constant and Beyond
• The effective theory of fluids at NLO and implications for dark energy
• Renormalization-group flow of the effective action of cosmological large-scale structures
• A novel null test for the $\Lambda$CDM model with growth-rate data
• The Effective Field Theory of Large-Scale Structure and Multi-tracer
• Probing Neutrino Hierarchy and Chirality via Wakes
• A model-independent fit to Planck and BICEP2 data
• Non-linear relativistic contributions to the cosmological weak-lensing convergence
• Spoon or slide? The non-linear matter power spectrum in the presence of massive neutrinos
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• BOSS full-shape analysis from the EFTofLSS with exact time dependence
• Probing Asymmetric Structures in the Outskirts of Galaxies
• Disentangling interacting dark energy cosmologies with the three-point correlation function
• Dark matter-baryons separation at the lowest mass scale: the Bullet Group
• Modified gravity and coupled quintessence
• Cosmological Effects of Scalar-Photon Couplings: Dark Energy and Varying-alpha Models
• Nonparametric reconstruction of the Om diagnostic to test LCDM
• Lensing convergence in galaxy clustering in LambdaCDM and beyond
• Using Cross-Correlations to Calibrate Lensing Source Redshift Distributions: Improving Cosmological Constraints from Upcoming Weak Lensing Surveys
• Dark energy survivals in massive gravity after GW170817: SO(3) invariant
• Gravitational Lenses as High-Resolution Telescopes
• Observational Constraints in Nonlocal Gravity: the Deser-Woodard Case
• Unbiased Cosmological Parameter Estimation from Emission Line Surveys with Interlopers
• Fitting and forecasting non-linear coupled dark energy
• An Accurate Fitting Function For Scale-dependent Growth Rate in Hu-Sawicki $f(R)$ Gravity
• Field-level inference of galaxy intrinsic alignment from the SDSS-III BOSS survey
• Gaugessence: a dark energy model with early time radiation-like equation of state
• Calibration of colour gradient bias in shear measurement using HST/CANDELS data
• UV-extending Ghost Inflation
• Lensing in the Geodesic Light-Cone coordinates and its (exact) illustration to an off-center observer in Lemaître-Tolman-Bondi models
• High Redshift Long Gamma-Ray Bursts Hubble Diagram as a Test of Basic Cosmological Relations
• Intrinsic alignments and 3d weak gravitational lensing
• Probing Modified Gravity with Atom-Interferometry: a Numerical Approach
• Analyzing clustering of astrophysical gravitational-wave sources: Luminosity-distance space distortions
• Dark sectors of the Universe: A Euclid survey approach
• Cosmological Perturbations and Invariant Observables in Geodesic Lightcone Coordinates
• A common explanation of the Hubble tension and anomalous cold spots in the CMB
• Redshift-space distortions of galaxies, clusters and AGN: testing how the accuracy of growth rate measurements depends on scales and sample selections
• Improving Fisher matrix forecasts for galaxy surveys: window function, bin cross-correlation, and bin redshift uncertainty
• General Modified Gravity With 21cm Intensity Mapping: Simulations and Forecast
• Generalized Proca and its Constraint Algebra
• LiteBIRD Science Goals and Forecasts: Improving Sensitivity to Inflationary Gravitational Waves with Multitracer Delensing
• Novel Adaptive softening for collisionless N-body simulations: Eliminating spurious halos
• Semi-analytic galaxy formation in early dark energy cosmologies
• Future constraints on the gravitational slip with the mass profiles of galaxy clusters
• Testing extended Jordan-Brans-Dicke theories with future cosmological observations
• Minimal plateau inflationary cosmologies and constraints from reheating
• Disformally Coupled Scalar Fields and Inspiralling Trajectories
• The Schrödinger-Poisson method for Large-Scale Structure
• Screenings in Modified Gravity: a perturbative approach
• Constraints on the growth rate using the observed galaxy power spectrum
• Cosmological parameter inference from galaxy clustering: The effect of the posterior distribution of the power spectrum
• Optimization of spectroscopic surveys for testing non-Gaussianity
• Spatial variations of the fine-structure constant in symmetron models
• Modelling the matter bispectrum at small scales in modified gravity
• A cosmological exclusion plot: Towards model-independent constraints on modified gravity from current and future growth rate data
• Litmus Test for Cosmic Hemispherical Asymmetry in the Cosmic Microwave Background B-mode polarization
• Estimating the weak-lensing rotation signal in radio cosmic shear surveys
• Ultra-light axions and the kinetic Sunyaev-Zel'dovich Effect
• Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- II. A case study for magnification bias and radio continuum surveys
• One simulation to have them all: performance of the Bias Assignment Method against N-body simulations
• The traces of anisotropic dark energy in light of Planck
• Study of Goldstone Inflation in the domain of Einstein-Gauss-Bonnet gravity
• Ultra-large-scale approximations and galaxy clustering: debiasing constraints on cosmological parameters
• Inadequacy of internal covariance estimation for super-sample covariance
• Beyond $\Lambda$CDM with HI intensity mapping: robustness of cosmological constraints in the presence of astrophysics
• Renormalization of Lagrangian bias via spectral parameters
• The CMB lensing bi-spectrum as a probe of modified gravity theories
• Constraining scalar-Gauss-Bonnet Inflation by Reheating, Unitarity and PLANCK
• Inflationary Predictions and Moduli Masses
• The cosmological evolution condition of the Planck constant in the varying speed of light models through adiabatic expansion
• How can we tell whether dark energy is composed by multiple fields?
• Measuring ISW with next-generation radio surveys
• Dynamics of Supersymmetric Chameleons
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• Cosmological parameter forecasts by a joint 2D tomographic approach to CMB and galaxy clustering
• The Cosmological Perturbation Theory on the Geodesic Light-Cone background
• Observable Predictions for Massive-Neutrino Cosmologies with Model-Independent Dark Energy
• Magnification bias as a novel probe for primordial magnetic fields
• Raytracing simulations of coupled dark energy models
• Spontaneous "Scalar-Vector Galileons" from "Weyl bi-Connection" model
• Modified Einstein versus Modified Euler for Dark Matter
• Light-Cone Observables and Gauge-Invariance in the Geodesic Light-Cone Formalism
• Improving cosmological parameter estimation with the future 21 cm observation from SKA
• Generalised model-independent characterisation of strong gravitational lenses V: reconstructing the lensing distance ratio by supernovae for a general Friedmann universe
• Lensing corrections to the $E_g(z)$ statistics from large scale structure
• Probing the constancy of the speed of light with future galaxy survey: the case of SKA and Euclid
• 3D weak lensing with spin wavelets on the ball
• The effective field theory of K-mouflage
• Two-loop power spectrum with full time- and scale-dependence and EFT corrections: impact of massive neutrinos and going beyond EdS
• The ages of stellar populations in a warm dark matter universe
• Arbitrarily coupled $p-$forms in cosmological backgrounds
• Mitigating the noise of DESI mocks using analytic control variates
• Model-independent constraints on modified gravity from current data and from the Euclid and SKA future surveys
• Baryon Acoustic Oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
• No need for dark matter in galaxy clusters within Galileon theory
• Can the degeneracies in the gravity sector be broken?
• Weak lensing probe of cubic Galileon model
• Dark D-Brane Cosmology: from background evolution to cosmological perturbations
• Constraints on a scale-dependent bias from galaxy clustering
• Measuring the cosmic expansion rate using 21-cm velocity acoustic oscillations
• The self similarity of weak lensing peaks
• Particlelike solutions in modified gravity: the Higgs monopole
• LADDER: Revisiting the Cosmic Distance Ladder with Deep Learning Approaches and Exploring its Applications
• Minimal Higgs inflation
• Structure formation in dark energy cosmologies described by PADE parameterization
• The sparkling Universe: a scenario for cosmic void motions
• Scale-dependent bias from multiple-field inflation
• On Scale-Dependent Cosmic Shear Systematic Effects
• Constraining the origin of stellar binary black hole mergers by detections of their lensed host galaxies and gravitational wave signals
• The BAHAMAS project: Effects of a running scalar spectral index on large-scale structure
• Combining gravitational lensing and gravitational redshift to measure the anisotropic stress with future galaxy surveys
• Designing an Optimal LSST Deep Drilling Program for Cosmology with Type Ia Supernovae
• Opening the reheating box in multifield inflation
• Recovering a redshift-extended VSL signal from galaxy surveys
• Linear and non-linear perturbations in dark energy models
• The Scales of Gravitational Lensing
• Cosmological evolution of viable models in the generalized scalar-tensor theory
• Determination of the abundance of cosmic matter via the cell count moments of the galaxy distribution (1)
• HEROES: The Hawaii eROSITA Ecliptic Pole Survey Catalog
• Chameleon Field Dynamics During Inflation
• Measuring the distortion of time with relativistic effects in large-scale structure
• Constraining dark sector perturbations I: cosmic shear and CMB lensing
• Optimal void finders in weak lensing maps
• Small field models with gravitational wave signature supported by CMB data
• The Impact of Anisotropic Redshift Distributions on Angular Clustering
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• Modelling the next-to-leading order matter three-point correlation function using FFTLog
• On the Three Primordial Numbers
• Parameter constraints from weak lensing tomography of galaxy shapes and cosmic microwave background fluctuations
• Towards a realistic model of quarks and leptons, leptonic CP violation and neutrinoless $\beta \beta$-decay
• Brightest Cluster Galaxies Are Statistically Special From $z=0.3$ to $z=1$
• Reconstruction of the null-test for the matter density perturbations
• Two new approaches to the anomalous limit of Brans-Dicke to Einstein gravity
• Dynamics of minimally coupled dark energy in spherical halos of dark matter
• Odd-parity stability of hairy black holes in $U(1)$ gauge-invariant scalar-vector-tensor theories
• Global properties of the growth index of matter inhomogeneities in the universe
• Semi-Analytic Galaxy Formation in Massive Neutrino Cosmologies
• Null tests of the concordance model in the era of Euclid and the SKA
• Perturbation theory for cosmologies with non-linear structure
• A theoretical estimate of intrinsic ellipticity bispectra induced by angular momenta alignments
• Post-Newtonian $\gamma$-like parameters and the gravitational slip in scalar-tensor and $f(R)$ theories
• Second-order cosmological perturbation theory and initial conditions for $N$-body simulations
• Constraining Majorana CP Phase in Precision Era of Cosmology and Double Beta Decay Experiment
• Probing the primordial Universe with 21-cm line from cosmic dawn/epoch of reionization
• Testing General Relativity with the Doppler magnification effect
• Measuring the surface mass density ellipticity of redMaPPer galaxy clusters using weak-lensing
• The impact of spurious shear on cosmological parameter estimates from weak lensing observables
• Constraining the growth of perturbations with lensing of supernovae
• Large-scale retrospective relative spectro-photometric self-calibration in space
• Consistency of nonlinear interacting ghost dark energy with recent observations
• A Relativistic view on large scale N-body simulations
• Combining spectroscopic and photometric surveys using angular cross-correlations I: Algorithm and modelling
• Neglecting Primordial non-Gaussianity Threatens Future Cosmological Experiment Accuracy
• The $n$-point streaming model: how velocities shape correlation functions in redshift space
• DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology
• Pairwise velocities in the "Running FLRW" cosmological model
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Weak Lensing Skew-Spectrum
• DESI Complete Calibration of the Color-Redshift Relation (DC3R2): Results from early DESI data
• The adhesion model as a field theory for cosmological clustering
• Global properties of the growth index: mathematical aspects and physical relevance
• Parameter inference and model comparison using theoretical predictions from noisy simulations
• On the phenomenology of extended Brans-Dicke Gravity
• The cosmological principle in theories with torsion: The case of Einstein-Cartan-Dirac-Maxwell gravity
• Developing a unified pipeline for large-scale structure data analysis with angular power spectra -- III. Implementing the multi-tracer technique to constrain neutrino masses
• Non-Gaussian Shape Discrimination with Spectroscopic Galaxy Surveys
• Imitating intrinsic alignments: A bias to the CMB lensing-galaxy shape cross-correlation power spectrum induced by the large-scale structure bispectrum
• The kinematic Sunyaev-Zel'dovich effect of the large-scale structure (II): the effect of modified gravity
• The Integrated Sachs-Wolfe Effect in the Bulk Viscous Dark Energy Model
• Test of the Equivalence Principle in the Dark Sector on Galactic Scales
• Gravitational wave source counts at high redshift and in models with extra dimensions
• Projection effects of large-scale structures on weak-lensing peak abundances
• New observational constraints on interacting dark energy using galaxy clusters virial equilibrium states
• Calibrating magnification bias for the $E_G$ statistic to test general relativity
• Probing modified gravity in cosmic filaments
• A first comparison of Kinetic Field Theory with Eulerian Standard Perturbation Theory
• Got plenty of nothing: cosmic voids as a probe of particle dark matter
• Measuring the BAO peak position with different galaxy selections
• Reconstructing CMB fluctuations and the mean reionization optical depth
• A thermodynamic point of view on dark energy models
• Dark energy reconstruction analysis with artificial neural networks: Application on simulated Supernova Ia data from Rubin Observatory
• Exploring neutrino interactions in light of present and upcoming galaxy surveys
• The Alcock Paczynski test with Baryon Acoustic Oscillations: systematic effects for future surveys
• Angular distribution of cosmological parameters as a probe of inhomogeneities: a kinematic parametrisation
• X-ray galaxy clusters abundance and mass temperature scaling
• Observational Constraints on Varying Alpha in $\Lambda (\alpha )$CDM Cosmology
• Dark-energy dependent test of general relativity at cosmological scales
• Cosmological framework for renormalization group extended gravity at the action level
• Quantum quenches during inflation
• Binary systems in Palatini-f(R) gravity
• Beyond Einstein's General Relativity
• Absence of solid angle deficit singularities in beyond-generalized Proca theories
• The galaxy bias at second order in general relativity with Non-Gaussian initial conditions
• New Interpretations of the Cosmological Preference for a Negative Neutrino Mass
• Gravitational lensing time delays with massive photons
• Semi-analytic galaxy formation in coupled dark energy cosmologies
• Simultaneous effect of Modified Gravity and Primordial Non-Gaussianity in Large Scale Structure Observations
• Cosmology and CPT violating neutrinos
• Multiple Field Inflation and Signatures of Heavy Physics in the CMB
• Probing interacting dark sector models with future weak lensing-informed galaxy cluster abundance constraints from SPT-3G and CMB-S4
• Towards an accurate model of small-scale redshift-space distortions in modified gravity
• Peculiar velocity measurement in a clumpy universe
• Parametrizing growth in dark energy and modified gravity models
• Relativistic Euler Equations in cosmologies with non-linear structures
• Simple numerical implementation of general dark energy models
• Constraining Warm Dark Matter with high-$z$ supernova lensing
• Spherical collapse in coupled quintessence with a $\Lambda$CDM background
• Non minimally coupled condensate cosmologies: matching observational data with phase space
• High-redshift cosmology with oxygen lines from H$\alpha$ surveys
• Study on the mapping of halo clustering from real space to redshift space
• A new generic evolution for $k$-essence dark energy with $w\approx -1$
• On Weak Lensing Shape Noise
• Towards the geometry of the universe from data
• Galaxy cluster constraints on the coupling to photons of low-mass scalars
• Noncommutative Universe and Chameleon Field Dynamics
• On the ISW-cluster cross-correlation in future surveys
• Constraining the mass-concentration relation through weak lensing peak function
• Hubble drift in Palatini $f(\mathcal{R})$-theories
• Quantification of the multi-streaming effect in Redshift Space Distortion
• Derivative couplings in massive bigravity
• A direct probe of cosmological power spectra of the peculiar velocity field and the gravitational lensing magnification from photometric redshift surveys
• Exploring the distance-redshift relation with gravitational wave standard sirens and tomographic weak lensing
• Screening vs. gevolution: in chase of a perfect cosmological simulation code
• Detectable Data-driven Features in the Primordial Scalar Power Spectrum
• Screening and degenerate kinetic self-acceleration from the nonlinear freedom of reconstructed Horndeski theories
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• The importance of the cosmic web and halo substructure for power spectra
• Primordial perturbations and inflation in holographic cosmology
• Effects of tidal gravitational fields in clustering dark energy models
• Angular distribution of cosmological parameters as a probe of space-time inhomogeneities
• Cosmological perturbations in the $\Lambda$CDM-like limit of a polytropic dark matter model
• Bayesian model selection for dark energy using weak lensing forecasts
• The Quest for the Inflationary Spectral Runnings in the Presence of Systematic Errors
• A Large Mass Hierarchy from a Small Non-minimal Coupling
• Spectroradiometry with Space Telescopes
• A covariant approach to parameterised cosmological perturbations
• The dark matter bispectrum from effective viscosity and one-particle irreducible vertices
• Galaxies as High-Resolution Telescopes
• Astrophysics with the Laser Interferometer Space Antenna
• Higher moments of primordial non-Gaussianity and N-body simulations
• Tidal shear and the consistency of microscopic Lagrangian halo approaches
• Baryon acoustic oscillations from HI intensity mapping: the importance of cross-correlations in the monopole and quadrupole
• Euclid preparation: VI. Verifying the Performance of Cosmic Shear Experiments
• On the consistency of the expansion with the perturbations
• The environment-dependence of the growth of the most massive objects in the Universe
• General Relativistic Effects in Weak Lensing Angular Power Spectra
• What We Can Learn from the Running of the Spectral Index if no Tensors are Detected in the Cosmic Microwave Background Anisotropy
• Cosmological cancellation of the vacuum energy density
• Unraveling the nature of Gravity through our clumpy Universe
• Mass - concentration relation and weak lensing peak counts
• Efficient implementation of the Time Renormalization Group
• Cosmic acceleration in screening hybrid quintessence model
• Small field models of inflation that predict a tensor-to-scalar ratio $r=0.03$
• Kinetic Field Theory applied to Vector-Tensor Gravity
• Impact of our local environment on cosmological statistics
• Probing Long-Range Forces Between Neutrinos with Cosmic Structures
• Ultra-local models of modified gravity without kinetic term
• Cosmology with sterile neutrino masses from oscillation experiments
• On the effect of projections on convergence peak counts and Minkowski functionals
• Can the homogeneity scale be used as a standard ruler?
• Non-standard hierarchies of the runnings of the spectral index in inflation
• Beyond boundaries of redshift surveys: assessing mass fluctuations on "super-survey" scales
• Breaking the Dark Degeneracy with the Drifting Coefficient of the Field Cluster Mass Function
• The Effects of Calibration on the Bias of Shear Measurements
• Warm and Cold Dark Matter in Bouncing Universe
• Neutrino Physics Now and in the Near Future
• Higher-Order Spectra of Weak Lensing Convergence Maps in Parameterized Theories of Modified Gravity
• Numerical implementation of the Cubic Galileon model in PINOCCHIO
• Inflation with mixed helicities and its observational imprint on CMB
• Imprints of dark matter-massive neutrino interaction in upcoming post-reionization and galaxy surveys
• Studying G-axion Inflation model in light of PLANCK
• Tidal virialization of dark matter haloes with clustering dark energy
• Implications of quantum gravity for dark matter in the brane-world scenario
• Heavy ion collisions and cosmology
• Role of Future SNIa Data from Rubin LSST in Reinvestigating Cosmological Models
• Sample variance in N--body simulations and impact on tomographic shear predictions
• Massive neutrinos in nonlinear large scale structure: A consistent perturbation theory
• What does the information paradox say about the universe?
• Detecting Relativistic Doppler in Galaxy Clustering with Tailored Galaxy Samples
• New- vs. chaotic-inflations
• Measuring lensing ratios with future cosmological surveys
• Model independent variance cancellation in CMB lensing cross-correlations
• Non-linear coupling in the dark sector as a running vacuum model
• Weakly Inhomogeneous models for the Low-Redshift Universe
• Unifying inflationary and reheating solution
• Speeding up the detectability of the harmonic-space galaxy bispectrum
• Mimicking the $\Lambda$CDM Universe through inhomogeneous space-time
• Observational effects of the early episodically dominating dark energy
• Spinning Guest Fields during Inflation: Leftover Signatures
• A new mechanism for dark energy: the adaptive screening
• Model-independent constraints on clustering and growth of cosmic structures from BOSS DR12 galaxies in harmonic space
• Detecting Relativistic Doppler by Multi-Tracing a Single Galaxy Population
• Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
• Are Cold Dynamical Dark Energy Models Distinguishable in the Light of the Data?
• UNITSIM-Galaxies: data release and clustering of emission-line galaxies
• The string theory swampland in the Euclid, SKA and Vera Rubin observatory era
• Quasilocal mass and multipole expansion in scalar-tensor gravity
• Stabilising the Planck mass shortly after inflation
• Constraining Recent Oscillations in Quintessence Models with Euclid
• Confronting global 21-cm signal with ${\mathbb{Z}}_3$ symmetric dark matter models
• Towards a Gravity Dual for the Large Scale Structure of the Universe
• Doubly coupled matter fields in massive bigravity
• The Large Scale Structure Bootstrap: perturbation theory and bias expansion from symmetries
• Can dark energy explain a high growth index?
• Qualitative probe of interacting dark energy with redshift-space distortions
• Dark Energy Simulations
• Probing Interacting Dark Sectors with upcoming Post-Reionization and Galaxy Surveys
• Illuminating the Dark Sector: Understanding Modified Gravity Signatures with Cross-Correlations of Gravitational Waves and Large-Scale Structure
• Perspectives for studying the dark energy at z>2 with galaxy surveys
• Generalized local ansatz for scale-dependent primordial non-Gaussianities and future galaxy surveys
• Non-linear structure formation in the "Running FLRW" cosmological model
• Weak lensing deflection of three-point correlation functions
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• Neutrino masses from CMB B-mode polarization and cosmic growth rate
• Impact of PSF misestimation and galaxy population bias on precision shear measurement using a CNN
• Implications of a high growth index on the variation of $G$
• Embedding the stationary spacetimes into Brans-Dicke cosmology via conformal transformations
• Constraining Quintessence Models with ISW-tSZ Cross-Correlations: A Comparative Analysis of Thawing, Tracker, and Scaling-Freezing Dynamics
• Towards simulating a realistic data analysis with an optimised angular power spectrum of spectroscopic galaxy surveys
• Stable Clustering Ansatz, Consistency Relations and Gravity Dual of Large-Scale Structure
• Dark energy model selection with current and future data
• Weak gravitational flexion in various spacetimes: Exotic lenses and modified gravity
• Growth Diagnostics for Dark Energy models and EUCLID forecast
• Dark energy and non-linear power spectrum
• The miniJPAS survey quasar selection I: Mock catalogues for classification
• Observational assessment of the viability of de Sitter-Gödel-de Sitter phase transition
• Improving cosmological covariance matrices with machine learning
• Investigating the Constraints on Primordial Features with Future Cosmic Microwave Background and Galaxy Surveys
• Semi-analytical Study on the Generic Degeneracy for Galaxy Clustering Measurements
• Fisher matrix for multiple tracers: the information in the cross-spectra