Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
arXiv:2010.15278 · doi:10.1103/PhysRevD.105.043522
Abstract
We provide an end-to-end exploration of a distinct modified gravitational theory in Jordan-Brans-Dicke (JBD) gravity, from an analytical and numerical description of the background expansion and linear perturbations, to the nonlinear regime captured with a hybrid suite of -body simulations, to the parameter constraints from existing cosmological probes. The nonlinear corrections to the matter power spectrum due to baryons, massive neutrinos, and modified gravity are simultaneously modeled and propagated in the cosmological analysis for the first time. In the combined analysis of the Planck CMB temperature, polarization, and lensing reconstruction, Pantheon supernova distances, BOSS measurements of BAO distances, the Alcock-Paczynski effect, and the growth rate, along with the joint (pt) dataset of cosmic shear, galaxy-galaxy lensing, and overlapping redshift-space galaxy clustering from KiDS and 2dFLenS, we constrain the JBD coupling constant, (95% CL), the effective gravitational constant, , the sum of neutrino masses, eV (95% CL), and the baryonic feedback amplitude, (95% CL), all in agreement with the standard model expectation. We show that the uncertainty in the gravitational theory alleviates the tension between KiDS2dFLenS and Planck to below and the tension in the Hubble constant between Planck and the direct measurement of Riess et al. (2019) down to ~; however, we find no substantial model selection preference for JBD gravity relative to CDM. We further show that the neutrino mass bound degrades by up to a factor of three as the parameterization becomes more restrictive and that a positive shift in suppresses the CMB damping tail in a way that might complicate future inferences of small-scale physics. (Abridged)
arXiv comment53 pages, 26 figures, results unchanged, version accepted for publication by PRD. Abstract abridged. Our MCMC chains, likelihood code, and data products are public at https://github.com/sjoudaki/CosmoJBD
References in corpus (195)
- Planck 2015 results. XIII. Cosmological parameters
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Planck 2013 results. XVI. Cosmological parameters
- Efficient Computation of CMB anisotropies in closed FRW models
- Modified Gravity and Cosmology
- f(R) theories
- Cosmological parameters from CMB and other data: a Monte-Carlo approach
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
- The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
- Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES
- Stable clustering, the halo model and nonlinear cosmological power spectra
- The Baryon Oscillation Spectroscopic Survey of SDSS-III
- Halo Models of Large Scale Structure
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples
- Coupled Quintessence
- The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
- Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
- Cosmological Perturbation Theory in the Synchronous vs. Conformal Newtonian Gauge
- Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space
- Chameleon Cosmology
- The Simons Observatory: Science goals and forecasts
- Testing General Relativity with Present and Future Astrophysical Observations
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
- Bayes in the sky: Bayesian inference and model selection in cosmology
- Bayesian photometric redshift estimation
- Revising the Halofit Model for the Nonlinear Matter Power Spectrum
- Planck 2018 results. V. CMB power spectra and likelihoods
- The Effective Field Theory of Inflation
- From k-essence to generalised Galileons
- Covariant Galileon
- Information criteria for astrophysical model selection
- KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing
- Big Bang Nucleosynthesis: 2015
- Dark Energy after GW170817: dead ends and the road ahead
- Cosmology and fundamental physics with the Euclid satellite
- The physics driving the cosmic star formation history
- Strong constraints on cosmological gravity from GW170817 and GRB 170817A
- Dark Energy after GW170817 and GRB170817A
- KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics
- Cosmic Growth History and Expansion History
- KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints
- Planck 2018 results. VIII. Gravitational lensing
- Varying constants, Gravitation and Cosmology
- Healthy theories beyond Horndeski
- Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters
- Symmetron Fields: Screening Long-Range Forces Through Local Symmetry Restoration
- Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear
- The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters
- Intrinsic alignment-lensing interference as a contaminant of cosmic shear
- Transforming gravity: from derivative couplings to matter to second-order scalar-tensor theories beyond the Horndeski Lagrangian
- The relativistic pulsar-white dwarf binary PSR J1738+0333 II. The most stringent test of scalar-tensor gravity
- Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
- The Effective Field Theory of Dark Energy
- The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9
- Dark energy constraints from cosmic shear power spectra: impact of intrinsic alignments on photometric redshift requirements
- Primordial Nucleosynthesis: from precision cosmology to fundamental physics
- Anisotropies in the Cosmic Microwave Background: An Analytic Approach
- Exploring gravitational theories beyond Horndeski
- The effects of galaxy formation on the matter power spectrum: A challenge for precision cosmology
- Gravitational Lensing Analysis of the Kilo Degree Survey
- An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models
- Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity
- The effects of He I 10830 on helium abundance determinations
- Degenerate higher order scalar-tensor theories beyond Horndeski up to cubic order
- A discriminating probe of gravity at cosmological scales
- Extended Scalar-Tensor Theories of Gravity
- Big-Bang Nucleosynthesis After Planck
- Dark Energy Survey Year 1 Results: Constraints on Extended Cosmological Models from Galaxy Clustering and Weak Lensing
- An introduction to the Vainshtein mechanism
- Interpreting large-scale redshift-space distortion measurements
- Signatures of Relativistic Neutrinos in CMB Anisotropy and Matter Clustering
- KiDS+VIKING-450: Cosmic shear tomography with optical+infrared data
- Solving Large Scale Structure in Ten Easy Steps with COLA
- Advanced ACTPol Cryogenic Detector Arrays and Readout
- Confirmation of general relativity on large scales from weak lensing and galaxy velocities
- Quantifying the effect of baryon physics on weak lensing tomography
- How Massless Neutrinos Affect the Cosmic Microwave Background Damping Tail
- Matter density perturbations and effective gravitational constant in modified gravity models of dark energy
- KiDS-450 + 2dFLenS: Cosmological parameter constraints from weak gravitational lensing tomography and overlapping redshift-space galaxy clustering
- A precision calculation of the effective number of cosmological neutrinos
- Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data
- CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics
- Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces
- The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at
- Observational Tests of Modified Gravity
- The Coyote Universe Extended: Precision Emulation of the Matter Power Spectrum
- Effective gravitational couplings for cosmological perturbations in the most general scalar-tensor theories with second-order field equations
- Effective Field Theory of Cosmic Acceleration: an implementation in CAMB
- Concordance and Discordance in Cosmology
- Prospects for resolving the Hubble constant tension with standard sirens
- Neutrino mass from Cosmology
- The Atacama Cosmology Telescope: Two-Season ACTPol Spectra and Parameters
- The Effect of Physical Assumptions on the Calculation of Microwave Background Anisotropies
- KiDS-450: Testing extensions to the standard cosmological model
- The BACCO Simulation Project: Exploiting the full power of large-scale structure for cosmology
- The Coyote Universe III: Simulation Suite and Precision Emulator for the Nonlinear Matter Power Spectrum
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale Structure Catalogs for Cosmological Analysis
- A New Nucleosynthesis Constraint on the Variation of G
- Current constraints on the cosmic growth history
- Quantifying baryon effects on the matter power spectrum and the weak lensing shear correlation
- Euclid preparation: II. The EuclidEmulator -- A tool to compute the cosmology dependence of the nonlinear matter power spectrum
- CFHTLenS: Testing the Laws of Gravity with Tomographic Weak Lensing and Redshift Space Distortions
- Modified Gravity-GADGET: A new code for cosmological hydrodynamical simulations of modified gravity models
- Testing General Relativity with Current Cosmological Data
- The BAHAMAS project: the CMB--large-scale structure tension and the roles of massive neutrinos and galaxy formation
- Modelling baryonic feedback for survey cosmology
- hi_class: Horndeski in the Cosmic Linear Anisotropy Solving System
- Effective Description of Higher-Order Scalar-Tensor Theories
- KiDS+VIKING-450 and DES-Y1 combined: Cosmology with cosmic shear
- Matter power spectrum and the challenge of percent accuracy
- Testing the universality of free fall by tracking a pulsar in a stellar triple system
- Measuring the effective complexity of cosmological models
- Constraints on a New Post-General Relativity Cosmological Parameter
- KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs
- The Observational Future of Cosmological Scalar-Tensor Theories
- Cosmic Degeneracies I: Joint N-body Simulations of Modified Gravity and Massive Neutrinos
- Cosmological constraints on Brans-Dicke theory
- Brans-Dicke gravity with a cosmological constant smoothes out CDM tensions
- On the road to percent accuracy: nonlinear reaction of the matter power spectrum to dark energy and modified gravity
- The response of primordial abundances to a general modification of and/or of the early universe expansion rate
- Scalar-tensor theories of gravity, neutrino physics, and the tension
- Modeling baryonic physics in future weak lensing surveys
- Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio
- What can Cosmology tell us about Gravity? Constraining Horndeski with Sigma and Mu
- The halo model as a versatile tool to predict intrinsic alignments
- Constraining The Early-Universe Baryon Density And Expansion Rate
- Bayesian evidence as a tool for comparing datasets
- Cosmic Microwave Background Temperature and Polarization Anisotropy in Brans-Dicke Cosmology
- Improved BBN Constraints on the Variation of the Gravitational Constant
- Gravity in the Era of Equality: Towards solutions to the Hubble problem without fine-tuned initial conditions
- Cosmic Shear Results from the Deep Lens Survey - II: Full Cosmological Parameter Constraints from Tomography
- COLA with scale-dependent growth: applications to screened modified gravity models
- Can we measure the neutrino mass hierarchy in the sky?
- Constraints on perfect fluid and scalar field dark energy models from future redshift surveys
- KiDS+GAMA: Intrinsic alignment model constraints for current and future weak lensing cosmology
- Cosmological parameter constraints for Horndeski scalar-tensor gravity
- Structure formation constraints on the Jordan-Brans-Dicke theory
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: theoretical systematics and Baryon Acoustic Oscillations in the galaxy correlation function
- A hydrodynamical halo model for weak-lensing cross correlations
- Cosmic microwave background with Brans-Dicke gravity II: constraints with the WMAP and SDSS data
- Baryonic effects for weak lensing. Part I. Power spectrum and covariance matrix
- The 2-degree Field Lensing Survey: design and clustering measurements
- RCSLenS: Testing gravitational physics through the cross-correlation of weak lensing and large-scale structure
- Constraints on the Variation of G from Primordial Nucleosynthesis
- WMAP constraints on scalar-tensor cosmology and the variation of the gravitational constant
- Probing the Friedmann equation during recombination with future CMB experiments
- Brans-Dicke cosmology with a - term: a possible solution to CDM tensions
- On the road to percent accuracy IV: ReACT -- computing the non-linear power spectrum beyond CDM
- The separate and combined effects of baryon physics and neutrino free-streaming on large-scale structure
- Is there concordance within the concordance CDM model?
- No Slip Gravity
- An improved test of the strong equivalence principle with the pulsar in a triple star system
- MGCAMB with massive neutrinos and dynamical dark energy
- CMB and BAO constraints for an induced gravity dark energy model with a quartic potential
- Weak Lensing Light-Cones in Modified Gravity simulations with and without Massive Neutrinos
- Cosmological discordances: a new measure, marginalization effects, and application to geometry vs growth current data sets
- KiDS+VIKING-450: Improved cosmological parameter constraints from redshift calibration with self-organising maps
- Model-independent constraints on the cosmological anisotropic stress
- Constraints on the Brans-Dicke gravity theory with the Planck data
- Cosmological constraints on induced gravity dark energy models
- The halo model in a massive neutrino cosmology
- KiDS+2dFLenS+GAMA: Testing the cosmological model with the statistic
- A comparison of Einstein-Boltzmann solvers for testing General Relativity
- KiDS+GAMA: Constraints on Horndeski gravity from combined large-scale structure probes
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity
- Extended quintessence with an exponential coupling
- The radiation-matter transition in Jordan-Brans-Dicke theory
- Baryonic effects for weak lensing. Part II. Combination with X-ray data and extended cosmologies
- Constraining Scalar-Tensor Modified Gravity with Gravitational Waves and Large Scale Structure Surveys
- Searching for Modified Gravity: Scale and Redshift Dependent Constraints from Galaxy Peculiar Velocities
- Planck constraints on scalar-tensor cosmology and the variation of the gravitational constant
- A Multi-Parameter Investigation of Gravitational Slip
- Consistency tests in cosmology using relative entropy
- The effect on cosmological parameter estimation of a parameter dependent covariance matrix
- Testing gravity using galaxy-galaxy lensing and clustering amplitudes in KiDS-1000, BOSS and 2dFLenS
- A Fast Route to Modified Gravitational Growth
- Quantifying Suspiciousness Within Correlated Data Sets
- Measuring gravity at cosmological scales
- Galaxy formation in the brane world I: overview and first results
- Quantifying Concordance in Cosmology
- Information Gains from Cosmological Probes
- Investigating the degeneracy between modified gravity and massive neutrinos with redshift-space distortions
- Testing gravity on cosmological scales with cosmic shear, cosmic microwave background anisotropies, and redshift-space distortions
- Cosmological constraints on scalar-tensor gravity and the variation of the gravitational constant
- J-PAS: forecasts on dark energy and modified gravity theories
- A new measure of tension between experiments
- Simulating galaxy formation in f(R) modified gravity: Matter, halo, and galaxy-statistics
- The phenomenology of beyond Horndeski gravity
- Testing extended Jordan-Brans-Dicke theories with future cosmological observations
- On the phenomenology of extended Brans-Dicke Gravity
- Cross-bispectra Constraints on Modified Gravity Theories from Nancy Grace Roman Space Telescope and Rubin Observatory Legacy Survey of Space and Time
- The Uncertainty in Newton's Constant and Precision Predictions of the Primordial Helium Abundance
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- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys
- Scant evidence for thawing quintessence
- The growth of density perturbations in the last 10 billion years from tomographic large-scale structure data
- A fast test to assess the impact of marginalization in Monte Carlo analyses, and its application to cosmology
- Can scale-dependent cosmology alleviate the tension?
- Positivity Bounds on Dark Energy: When Matter Matters
- Cosmological constraints on the gravitational constant
- Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
- Fast and accurate predictions of the nonlinear matter power spectrum for general models of Dark Energy and Modified Gravity
- First-order thermodynamics of scalar-tensor cosmology
- Scalar Fields Near Compact Objects: Resummation versus UV Completion
- Constraints on self-interacting Bose-Einstein condensate dark matter using large-scale observables
- Scalar-Tensor Gravity and DESI 2024 BAO data
- Testing the Speed of Gravity with Black Hole Ringdown
- Euclid: Constraining linearly scale-independent modifications of gravity with the spectroscopic and photometric primary probes
- Type Ia supernovae data with scalar-tensor gravity
- Constraints on and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering
- Sesame: A power spectrum emulator pipeline for beyond-CDM models
- Cosmological Tests of Gravity: A Future Perspective
- On tachyonic stability priors for dark energy
- Dynamics of self-gravitating systems in non-linearly magnetized chameleonic Brans-Dicke gravity
- Special Issue on Modified Gravity Approaches to the Tensions of CDM: Goals and Highlights
- Particle Production Scenario in an Algebraically Coupled Quintessence Field with a Dark Matter Fluid
- 6x2pt: Forecasting gains from joint weak lensing and galaxy clustering analyses with spectroscopic-photometric galaxy cross-correlations
- A simple prediction of the nonlinear matter power spectrum in Brans-Dicke gravity from linear theory
- Toward testing gravity with LSST using
- A New Approach to Flatness, Horizon and Late-time Accelerating Expansion Problems on the basis of Mach Principle