New tests of dark sector interactions from the full-shape galaxy power spectrum

Abstract

We explore the role of redshift-space galaxy clustering data in constraining non-gravitational interactions between dark energy (DE) and dark matter (DM), for which state-of-the-art limits have so far been obtained from late-time background measurements. We use the joint likelihood for pre-reconstruction full-shape (FS) galaxy power spectrum and post-reconstruction Baryon Acoustic Oscillation (BAO) measurements from the BOSS DR12 sample, alongside Cosmic Microwave Background (CMB) data from \textit{Planck}: from this dataset combination we infer $H_0=68.02_{-0.60}^{+0.49}\mathrm{km}/\mathrm{s}/\mathrm{Mpc}$ and the 2$\sigma$ lower limit $\xi >-0.12$, among the strongest limits ever reported on the DM-DE coupling strength $\xi$ for the particular model considered. Contrary to what has been observed for the $\Lambda$CDM model and simple extensions thereof, we find that the CMB+FS combination returns tighter constraints compared to the CMB+BAO one, suggesting that there is valuable additional information contained in the broadband of the power spectrum. We test this finding by running additional CMB-free analyses and removing sound horizon information, and discuss the important role of the equality scale in setting constraints on DM-DE interactions. Our results reinforce the critical role played by redshift-space galaxy clustering measurements in the epoch of precision cosmology, particularly in relation to tests of non-minimal dark sector extensions of the $\Lambda$CDM model.

arXiv comment18 Pages, 4 Figures, 2 Tables. Matches the version published in PRD

References in corpus (309)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• Cosmological Imprint of an Energy Component with General Equation of State
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• Cosmology and the Fate of Dilatation Symmetry
• Quintessence, Cosmic Coincidence, and the Cosmological Constant
• The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
• In the Realm of the Hubble tension $-$ a Review of Solutions
• Coupled Quintessence
• The Simons Observatory: Science goals and forecasts
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
• Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• Quintessence and the Rest of the World
• Planck 2018 results. V. CMB power spectra and likelihoods
• Cosmology and Fundamental Physics with the Euclid Satellite
• Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code
• KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics
• Planck 2018 results. VIII. Gravitational lensing
• The trouble with $H_0$
• The Hubble Hunter's Guide
• Cosmological Non-Linearities as an Effective Fluid
• The Effective Field Theory of Cosmological Large Scale Structures
• The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Cosmology Intertwined II: The Hubble Constant Tension
• Renormalized Cosmological Perturbation Theory
• New physics in light of the $H_0$ tension: an alternative view
• Improving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak
• Dynamical dark energy in light of the latest observations
• Interacting Dark Matter and Dark Energy
• The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
• Cosmological Parameters from the BOSS Galaxy Power Spectrum
• Non-minimal dark sector physics and cosmological tensions
• Can interacting dark energy solve the $H_0$ tension?
• Baryon Acoustic Oscillations in 2D: Modeling Redshift-space Power Spectrum from Perturbation Theory
• Unveiling $\nu$ secrets with cosmological data: neutrino masses and mass hierarchy
• Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
• Large-scale instability in interacting dark energy and dark matter fluids
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space
• Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• Early Dark Energy Does Not Restore Cosmological Concordance
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0
• Aspects of the cosmological "coincidence problem"
• How Massless Neutrinos Affect the Cosmic Microwave Background Damping Tail
• Does the Hubble constant tension call for new physics?
• Evidence for a non-zero Lambda and a low matter density from a combined analysis of the 2dF Galaxy Redshift Survey and Cosmic Microwave Background Anisotropies
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in Fourier-space
• Measurements of the E-Mode Polarization and Temperature-E-Mode Correlation of the CMB from SPT-3G 2018 Data
• To H0 or not to H0?
• Tracking and coupled dark energy as seen by WMAP
• Nonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian picture
• The IR-resummed Effective Field Theory of Large Scale Structures
• Constraining Early Dark Energy with Large-Scale Structure
• Cosmologies with Energy Exchange
• Effects of the interaction between dark energy and dark matter on cosmological parameters
• Resolving the Hubble Tension with New Early Dark Energy
• Elucidating $\Lambda$CDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy
• Sounds Discordant: Classical Distance Ladder & $\Lambda$CDM -based Determinations of the Cosmological Sound Horizon
• Thermodynamics of dark energy interacting with dark matter and radiation
• Constraints on the sum of the neutrino masses in dynamical dark energy models with $w(z)\ge -1$ are tighter than those obtained in $\Lambda$CDM
• Convolution Lagrangian perturbation theory for biased tracers
• Echo of interactions in the dark sector
• Probing the interaction between dark matter and dark energy in the presence of massive neutrinos
• Hydrodynamical N-body simulations of coupled dark energy cosmologies
• Non-linear perturbation theory extension of the Boltzmann code CLASS
• Equivalence Principle and the Baryon Acoustic Peak
• Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension
• Reconciling CMB and structure growth measurements with dark energy interactions
• Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0
• Bias in the Effective Field Theory of Large Scale Structures
• Hubble Sinks In The Low-Redshift Swampland
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the configuration-space clustering wedges
• Consistency tests of $\Lambda$CDM from the early integrated Sachs-Wolfe effect: Implications for early-time new physics and the Hubble tension
• The Lagrangian-space Effective Field Theory of Large Scale Structures
• Dark coupling
• Loop Corrections in Non-Linear Cosmological Perturbation Theory
• Time-Sliced Perturbation Theory II: Baryon Acoustic Oscillations and Infrared Resummation
• Biased Tracers and Time Evolution
• Interacting dark energy with time varying equation of state and the $H_0$ tension
• Revisiting a negative cosmological constant from low-redshift data
• Coupled and Extended Quintessence: theoretical differences and structure formation
• The Effective Field Theory of Large Scale Structures at Two Loops
• Does Hubble Tension Signal a Breakdown in FLRW Cosmology?
• A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO
• On the improvement of cosmological neutrino mass bounds
• Cosmology from large-scale structure: Constraining $\Lambda$CDM with BOSS
• Multi-Point Propagators in Cosmological Gravitational Instability
• Early dark energy is not excluded by current large-scale structure data
• On the Renormalization of the Effective Field Theory of Large Scale Structures
• Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum
• Efficient Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
• Can the $H_0$ tension be resolved in extensions to $\Lambda$CDM cosmology?
• Update on Coupled Dark Energy and the $H_0$ tension
• Limits on $w$CDM from the EFTofLSS with the PyBird code
• New constraints on interacting dark energy from cosmic chronometers
• Cosmological Parameters and Neutrino Masses from the Final Planck and Full-Shape BOSS Data
• The Bispectrum in the Effective Field Theory of Large Scale Structure
• Dark sector interaction: a remedy of the tensions between CMB and LSS data
• Models of coupled dark matter to dark energy
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: structure growth rate measurement from the anisotropic quasar power spectrum in the redshift range $0.8<z<2.2$
• A combined analysis of the $H_0$ late time direct measurements and the impact on the Dark Energy sector
• The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data
• Early modified gravity in light of the $H_0$ tension and LSS data
• Cosmological parameters from large scale structure - geometric versus shape information
• Redshift-Space Distortions in Lagrangian Perturbation Theory
• Constraints on the Coupling between Dark Energy and Dark Matter from CMB data
• The Shift of the Baryon Acoustic Oscillation Scale: A Simple Physical Picture
• Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions
• Consistent Modeling of Velocity Statistics and Redshift-Space Distortions in One-Loop Perturbation Theory
• The Effective Field Theory of Large Scale Structure at Two Loops: the apparent scale dependence of the speed of sound
• New constraint on Early Dark Energy from Planck and BOSS data using the profile likelihood
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the Fourier space wedges of the final sample
• The galaxy power spectrum take on spatial curvature and cosmic concordance
• Coupled quintessence and the coincidence problem
• Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder
• Interacting Quintessence, Cosmic Acceleration and the Coincidence Problem
• Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models
• Observational constraints on sign-changeable interaction models and alleviation of the $H_0$ tension
• Constraints on the interacting vacuum -- geodesic CDM scenario
• Adiabatic instability in coupled dark energy-dark matter models
• A Consistent Effective Theory of Long-Wavelength Cosmological Perturbations
• Dark Energy at early times and ACT: a larger Hubble constant without late-time priors
• Coupled dark matter-dark energy in light of near Universe observations
• The Parameterized Post-Friedmannian Framework for Interacting Dark Energy Theories
• Adiabatic initial conditions for perturbations in interacting dark energy models
• Perturbations in a coupled scalar field cosmology
• Cosmological Perturbation Theory Using the FFTLog: Formalism and Connection to QFT Loop Integrals
• Galaxy Bias and Primordial Non-Gaussianity
• The One-Loop Matter Bispectrum in the Effective Field Theory of Large Scale Structures
• Scale-dependent galaxy bias, CMB lensing-galaxy cross-correlation, and neutrino masses
• Analytic Prediction of Baryonic Effects from the EFT of Large Scale Structures
• The 2-loop matter power spectrum and the IR-safe integrand
• Testing modified gravity with Planck: the case of coupled dark energy
• Constraints on the curvature of the Universe and dynamical dark energy from the Full-shape and BAO data
• Cosmological dynamics of mimetic gravity
• Cosmological constraints from BOSS with analytic covariance matrices
• The Gaussian streaming model and Lagrangian effective field theory
• Field theoretic interpretations of interacting dark energy scenarios and recent observations
• Novel approach towards the large-scale stable Interacting Dark-Energy models and their Astronomical Bounds
• On the Velocity in the Effective Field Theory of Large Scale Structures
• Precision Comparison of the Power Spectrum in the EFTofLSS with Simulations
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
• 2021-$H_0$ Odyssey: Closed, Phantom and Interacting Dark Energy Cosmologies
• Evidence for interacting dark energy from BOSS
• Cosmic dissonance: new physics or systematics behind a short sound horizon?
• Parametrized Post-Friedmann Framework for Interacting Dark Energy
• On phenomenological models of dark energy interacting with dark matter
• Interacting Dark Energy in a closed universe
• On the EFT of Large Scale Structures in Redshift Space
• Dark calling Dark: Interaction in the dark sector in presence of neutrino properties after Planck CMB final release
• Precision analysis of the redshift-space galaxy bispectrum
• Dark Coupling and Gauge Invariance
• Relieving the $H_0$ tension with a new interacting dark energy model
• Cosmology in the era of Euclid and the Square Kilometre Array
• Implication of the Hubble tension for the primordial Universe in light of recent cosmological data
• Effective Theory of Large-Scale Structure with Primordial Non-Gaussianity
• Dark sectors with dynamical coupling
• New Early Dark Energy is compatible with current LSS data
• ShapeFit: extracting the power spectrum shape information in galaxy surveys beyond BAO and RSD
• Dark sector interaction and the supernova absolute magnitude tension
• Determining the Hubble Constant without the Sound Horizon: Measurements from Galaxy Surveys
• Exploring the full parameter space for an interacting dark energy model with recent observations including redshift-space distortions: Application of the parametrized post-Friedmann approach
• All-inclusive interacting dark sector cosmologies
• Quantum Field Theory of Interacting Dark Matter/Dark Energy: Dark Monodromies
• Constraints on coupled dark energy using CMB data from WMAP and SPT
• Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis
• Direct detection of dark energy: the XENON1T excess and future prospects
• Can dark energy be dynamical?
• Covariantizing the interaction between dark energy and dark matter
• Non-Gaussian Covariance of the Matter Power Spectrum in the Effective Field Theory of Large Scale Structure
• On the IR-Resummation in the EFTofLSS
• On the reach of perturbative descriptions for dark matter displacement fields
• Cosmological perturbation theory in 1+1 dimensions
• Constructing Regularized Cosmic Propagators
• Dark Sector to Restore Cosmological Concordance
• Coupled quintessence with a $\Lambda$CDM background: removing the ${\sigma }_8$ tension
• Bias due to neutrinos must not uncorrect'd go
• Systematic Renormalization of the Effective Theory of Large Scale Structure
• Cosmological constraints on parametrized interacting dark energy
• Single-Field Consistency Relations of Large Scale Structure. Part II: Resummation and Redshift Space
• On the Statistics of Biased Tracers in the Effective Field Theory of Large Scale Structures
• Cosmological constraints from the power spectrum of eBOSS emission line galaxies
• No-go guide for the Hubble tension : Late-time solutions
• The Trispectrum in the Effective Field Theory of Large Scale Structure
• Measurements of $H_0$ and reconstruction of the dark energy properties from a model-independent joint analysis
• Soundness of Dark Energy properties
• Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
• Looking for interactions in the cosmological dark sector
• Optimizing large-scale structure data analysis with the theoretical error likelihood
• Scalar-field dark energy nonminimally and kinetically coupled to dark matter
• Cosmological Measurements from Angular Power Spectra Analysis of BOSS DR12 Tomography
• Cosmological constraints without fingers of God
• Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing
• Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
• Constraints on interacting dark energy models through cosmic chronometers and Gaussian process
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• Dark Energy and Modified Gravity in the Effective Field Theory of Large-Scale Structure
• Testing AdS early dark energy with Planck, SPTpol and LSS data
• High-z massive clusters as a test for dynamical coupled dark energy
• Joint analysis of anisotropic power spectrum, bispectrum and trispectrum: application to N-body simulations
• An analytic implementation of the IR-resummation for the BAO peak
• Extended quintessence with an exponential coupling
• The latitude dependence of the rotation measures of NVSS sources
• Early massive clusters and the bouncing coupled dark energy
• Extending the modeling of the anisotropic galaxy power spectrum to $k=0.4h{\mathrm{Mpc}}^{-1}$
• Observational constraints on dark matter-dark energy scattering cross section
• Accurate emulator for the redshift-space power spectrum of dark matter halos and its application to galaxy power spectrum
• Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter
• Probing elastic interactions in the dark sector and the role of $S_8$
• Interacting Dark Energy: Possible Explanation for 21-cm Absorption at Cosmic Dawn
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• Understanding the suppression of structure formation from dark matter$\unicode{x2013}$dark energy momentum coupling
• Probing the imprint of interacting dark energy on very large scales
• The Effective Field Theory of Large Scale Structure at Three Loops
• Very Massive Tracers and Higher Derivative Biases
• Towards Precision Constraints on Gravity with the Effective Field Theory of Large-Scale Structure
• The EFT of Large Scale Structures at All Redshifts: Analytical Predictions for Lensing
• A fake Interacting Dark Energy detection?
• Maximal compression of the redshift space galaxy power spectrum and bispectrum
• Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy
• IR-safe and UV-safe integrands in the EFTofLSS with exact time dependence
• Future CMB cosmological constraints in a dark coupled universe
• Probing the interaction between dark energy and dark matter with the parametrized post-Friedmann approach
• Geometrization of light bending and its application to SdSw spacetime
• Interacting Diffusive Unified Dark Energy and Dark Matter from Scalar Fields
• Matter trispectrum: theoretical modelling and comparison to N-body simulations
• Multi-interacting dark energy and its cosmological implications
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• Exploring Early Dark Energy solution to the Hubble tension with Planck and SPTPol data
• Testing interacting dark matter and dark energy model with cosmological data
• Biased Tracers in Redshift Space in the EFTofLSS with exact time dependence
• Null test for interactions in the dark sector
• Probing the imprints of generalized interacting dark energy on the growth of perturbations
• Scaling solutions and weak gravity in dark energy with energy and momentum couplings
• Constraints on Pre-Recombination Early Dark Energy from SPT-3G Public Data
• Unified Dark Energy and Dark Matter from Dynamical Space Time
• Reconstruction of the Dark Energy equation of state from latest data: the impact of theoretical priors
• Dynamical Dark sectors and Neutrino masses and abundances
• Dark energy interactions near the galactic centre
• Cosmological constraints from a joint analysis of cosmic microwave background and spectroscopic tracers of the large-scale structure
• Exacerbating the cosmological constant problem with interacting dark energy
• Tree-Level Bispectrum in the Effective Field Theory of Large-Scale Structure extended to Massive Neutrinos
• Cosmology beyond BAO from the 3D distribution of the Lyman-$\alpha$ forest
• Determining the Hubble Constant without the Sound Horizon: Perspectives with Future Galaxy Surveys
• Future weak lensing constraints in a dark coupled universe
• Scaling solutions in scalar-tensor cosmologies
• An effective description of dark matter and dark energy in the mildly non-linear regime
• On the reach of perturbative methods for dark matter density fields
• Efficient exploration of cosmology dependence in the EFT of LSS
• Unification of DE-DM from Diffusive Cosmology
• Direct Probe of Dark Energy through Gravitational Lensing Effect
• On the Bispectra of Very Massive Tracers in the Effective Field Theory of Large-Scale Structure
• Probing the sign-changeable interaction between dark energy and dark matter with current observations
• Dark Energy coupling with electromagnetism as seen from future low-medium redshift probes
• A Fully Self-Consistent Cosmological Simulation Pipeline for Interacting Dark Energy Models
• Theoretical and observational bounds on some interacting vacuum energy scenarios
• Model-independent versus model-dependent interpretation of the SDSS-III BOSS power spectrum: Bridging the divide
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• Dark sector interactions and the curvature of the Universe in light of Planck's 2018 data
• Exploring dark matter microphysics with galaxy surveys
• Geometrical compression: a new method to enhance the BOSS galaxy bispectrum monopole constraints
• Dark Matter Halos in Interacting Dark Energy Models: Formation History, Density Profile, Spin and Shape
• On cosmological signatures of baryons-dark energy elastic couplings
• Precise Calibration of the One-Loop Bispectrum in the Effective Field Theory of Large Scale Structure
• Maps of CMB lensing deflection from N-body simulations in Coupled Dark Energy Cosmologies
• Consistency relations for large-scale structure in modified gravity and the matter bispectrum
• Constraints on the Early and Late Integrated Sachs-Wolfe effects from Planck 2015 Cosmic Microwave Background Anisotropies angular power spectra
• The two-loop bispectrum of large-scale structure
• Latest evidence for a late time vacuum -- geodesic CDM interaction
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Cosmological singularities in interacting dark energy models with an $\omega (q)$ parametrization
• Perturbation theory challenge for cosmological parameters estimation: Matter power spectrum in real space
• Principal Shapes and Squeezed Limits in the Effective Field Theory of Large Scale Structure
• Euclid: constraining dark energy coupled to electromagnetism using astrophysical and laboratory data
• J-PAS: Forecasts for dark matter - dark energy elastic couplings
• Constraining the dark-energy equation of state with cosmological data
• Dark energy and Dark matter interaction in light of the second law of thermodynamics
• Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids
• Probing Interacting Dark Energy and Scattering of Baryons with Dark Matter in Light of EDGES 21cm Signal
• Precise Calibration of the One-Loop Trispectrum in the Effective Field Theory of Large Scale Structure
• The first constraint from SDSS galaxy-galaxy weak lensing measurements on interacting dark energy models
• J-PAS: forecasts on interacting vacuum energy models
• Violation of the consistency relations for large-scale structure with dark energy
• Fine-structure constant constraints on dark energy
• Hubble constant and sound horizon from the late-time Universe
• Impact of bias and redshift-space modelling for the halo power spectrum: Testing the effective field theory of large-scale structure
• Fine-structure constant constraints on dark energy: II. Extending the parameter space
• Imprints of interacting dark energy on cosmological perturbations
• KiDS-1000 Cosmology: machine learning -- accelerated constraints on Interacting Dark Energy with COSMOPOWER
• Cosmological perturbations and dynamical analysis for interacting quintessence
• Modelling Non-Linear Effects of Dark Energy
• Linear Perturbation constraints on Multi-coupled Dark Energy
• Constraining coupled quintessence with the 21cm signal
• Coupling dark energy to dark matter inhomogeneities
• Differentiating dark interactions with perturbation
• Deconstructing the Planck TT Power Spectrum to Constrain Deviations from $\Lambda$CDM
• Dark energy and Equivalence Principle constraints from astrophysical tests of the stability of the fine-structure constant
• A test of the standard dark matter density evolution law using galaxy clusters and cosmic chronometers
• Supernova constraints on Multi-coupled Dark Energy
• Unphysical properties in a class of interacting dark energy models
• Constraints on interacting dynamical dark energy and a new test for $\Lambda$CDM
• Assessing non-linear models for galaxy clustering II: model validation and forecasts for Stage IV surveys
• Shan--Chen interacting vacuum cosmology
• Assessing non-linear models for galaxy clustering III: Theoretical accuracy for Stage IV surveys
• Probing the dark matter density evolution law with large scale structures
• $\Lambda$CDM as a Noether Symmetry in Cosmology
• Interacting dark energy from redshift-space galaxy clustering