Integrated Sachs-Wolfe effect in massive bigravity
arXiv:1501.02140 · doi:10.1103/PhysRevD.91.084046
Abstract
We study the integrated Sachs-Wolfe (ISW) effect in ghost-free, massive bigravity. We focus on the infinite-branch bigravity (IBB) model which exhibits viable cosmic expansion histories and stable linear perturbations, while the cosmological constant is set to zero and the late-time accelerated expansion of the Universe is due solely to the gravitational interaction terms. The ISW contribution to the CMB auto-correlation power spectrum is predicted, as well as the cross-correlation between the CMB temperature anisotropies and large-scale structure. We use ISW amplitudes as observed by the WMAP 9-year temperature data together with galaxy and AGN data provided by the WISE mission in order to compare the theoretical predictions to the observations. The ISW amplitudes in IBB are found to be larger than the corresponding ones in the standard LCDM model by roughly a factor of 1.5, but are still consistent with the observations.
10 pages, 3 figures. v2: refs added, minor rephrasings, results and conclusions unchanged. v3: matches version published in PRD
References in corpus (92)
- The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
- Resummation of Massive Gravity
- Generalization of the Fierz-Pauli Action
- Massive Gravity
- Bimetric Gravity from Ghost-free Massive Gravity
- Resolving the Ghost Problem in non-Linear Massive Gravity
- Confirmation of the Secondary Constraint and Absence of Ghost in Massive Gravity and Bimetric Gravity
- Ghost-free Massive Gravity with a General Reference Metric
- Planck 2013 results. XVII. Gravitational lensing by large-scale structure
- On Non-Linear Actions for Massive Gravity
- A correlation of the cosmic microwave sky with large scale structure
- Massive Cosmologies
- Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological Implications
- Looking for with the Rees-Sciama Effect
- An Imprint of Super-Structures on the Microwave Background due to the Integrated Sachs-Wolfe Effect
- Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications
- Ghost free Massive Gravity in the Stückelberg language
- Massive gravity: nonlinear instability of the homogeneous and isotropic universe
- Detection of the ISW and SZ effects from the CMB-Galaxy correlation
- Cross-Correlation of the Cosmic Microwave Background with the 2MASS Galaxy Survey: Signatures of Dark Energy, Hot Gas, and Point Sources
- Open FRW universes and self-acceleration from nonlinear massive gravity
- Cosmological Solutions in Bimetric Gravity and their Observational Tests
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Dark Energy Induced Correlation with Radio Sources
- Integrated Sachs-Wolfe effect from the cross correlation of WMAP3 year and the NRAO VLA sky survey data: New results and constraints on dark energy
- Cosmological solutions with massive gravitons in the bigravity theory
- Characterizing the Mid-IR Extragalactic Sky with WISE and SDSS
- Accelerated expansion from ghost-free bigravity: a statistical analysis with improved generality
- FRW Cosmology in Ghost Free Massive Gravity
- Cosmological perturbations of self-accelerating universe in nonlinear massive gravity
- Perturbations in Massive Gravity Cosmology
- On couplings to matter in massive (bi-)gravity
- Planck 2013 results. XIX. The integrated Sachs-Wolfe effect
- Helicity Decomposition of Ghost-free Massive Gravity
- Quasi-Dilaton: Theory and Cosmology
- Stable and unstable cosmological models in bimetric massive gravity
- Cosmological Stability Bound in Massive Gravity and Bigravity
- Measurement of the gravitational potential evolution from the cross-correlation between WMAP and the APM Galaxy survey
- Improved Primordial Non-Gaussianity Constraints from Measurements of Galaxy Clustering and the Integrated Sachs-Wolfe Effect
- Cosmological perturbations in Massive Gravity and the Higuchi bound
- Cross-correlation of the CMB and radio galaxies in real, harmonic and wavelet spaces: detection of the integrated Sachs-Wolfe effect and dark energy constraints
- Ghosts & Matter Couplings in Massive (bi-&multi-)Gravity
- Self-accelerating Massive Gravity: Exact solutions for any isotropic matter distribution
- Cross-correlation of WMAP 3rd year and the SDSS DR4 galaxy survey: new evidence for Dark Energy
- Integrated Sachs-Wolfe effect in Cross-Correlation: The Observer's Manual
- Nonlinear stability of cosmological solutions in massive gravity
- Mass-Varying Massive Gravity
- Correlating the CMB with Luminous Red Galaxies : The Integrated Sachs-Wolfe Effect
- Growth Histories in Bimetric Massive Gravity
- The significance of the integrated Sachs-Wolfe effect revisited
- A non-local theory of massive gravity
- Bimetric gravity doubly coupled to matter: theory and cosmological implications
- Exact self-accelerating cosmologies in the ghost-free bigravity and massive gravity
- A Possible Cold Imprint of Voids on the Microwave Background Radiation
- A direct measurement of the linear bias of mid-infrared-selected quasars at z~1 using cosmic microwave background lensing
- Cross-correlation of 2MASS and WMAP3: Implications for the Integrated Sachs-Wolfe effect
- Viable cosmology in bimetric theory
- Viable cosmological solutions in massive bimetric gravity
- Exact self-accelerating cosmologies in the ghost-free massive gravity -- the detailed derivation
- Cosmological perturbations in massive bigravity
- The integrated Sachs-Wolfe imprints of cosmic superstructures: a problem for ΛCDM
- FRW Cosmological Perturbations in Massive Bigravity
- The coupling to matter in Massive, Bi- and Multi-Gravity
- Cosmic expansion histories in massive bigravity with symmetric matter coupling
- The nature of spacetime in bigravity: two metrics or none?
- Cosmological dynamics and dark energy from non-local infrared modifications of gravity
- Instability in a minimal bimetric gravity model
- The Cosmology of Interacting Spin-2 Fields
- The stacked ISW signal of rare superstructures in ΛCDM
- Measuring the Integrated Sachs-Wolfe Effect
- Appearance of Boulware-Deser ghost in bigravity with doubly coupled matter
- Linear growth of structure in massive bigravity
- ISW measurements with photometric redshift surveys: 2MASS results and future prospects
- Multi-Metric Gravity via Massive Gravity
- Cosmological perturbations in massive gravity with doubly coupled matter
- Massive cosmological scalar perturbations
- Classical and quantum massive cosmology for the open FRW universe
- Cross-correlating WMAP5 with 1.5 million LRGs: a new test for the ISW effect
- The Jubilee ISW Project II: observed and simulated imprints of voids and superclusters on the cosmic microwave background
- Probing dark energy with steerable wavelets through correlation of WMAP and NVSS local morphological measures
- Integrated Sachs Wolfe Effect and Rees Sciama Effect
- Mass eigenstates in bimetric theory with matter coupling
- Weak Massive Gravity
- The SDSS-III Baryonic Oscillation Spectroscopic Survey: Constraints on the Integrated Sachs Wolfe effect
- Strong lensing constraints on bimetric massive gravity
- Cosmology in General Massive Gravity Theories
- Cross-correlation of WISE Galaxies with the Cosmic Microwave Background
- Selfacceleration with Quasidilaton
- An optimal estimator for the CMB-LSS angular power spectrum and its application to WMAP and NVSS data
- Cross-correlation of WMAP7 and the WISE Full Data Release
- Gaussian Approximation of Peak Values in the Integrated Sachs-Wolfe Effect
- Sunyaev-Zeldovich effect in WMAP and its effect on cosmological parameters
Cited by in corpus (33)
- Cosmology and Fundamental Physics with the Euclid Satellite
- Beyond CDM: Problems, solutions, and the road ahead
- Testing General Relativity in Cosmology
- A systematic approach to generalisations of General Relativity and their cosmological implications
- Galileon Gravity in Light of ISW, CMB, BAO and data
- Bimetric gravity is cosmologically viable
- Recent developments in bimetric theory
- The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
- Cosmology in bimetric theory with an effective composite coupling to matter
- Higuchi Ghosts and Gradient Instabilities in Bimetric Gravity
- Gravity at the horizon: on relativistic effects, CMB-LSS correlations and ultra-large scales in Horndeski's theory
- Neutron star merger GW170817 strongly constrains doubly coupled bigravity
- Galaxy cluster lensing masses in modified lensing potentials
- Dipolar Dark Matter with Massive Bigravity
- Mild bounds on bigravity from primordial gravitational waves
- On stars, galaxies and black holes in massive bigravity
- Scalar instabilities in bimetric gravity: The Vainshtein mechanism and structure formation
- Narrowing down the possible explanations of cosmic acceleration with geometric probes
- New massive bigravity cosmologies with double matter coupling
- Surfing gravitational waves: can bigravity survive growing tensor modes?
- Tensor Modes in Bigravity: Primordial to Present
- Consistent metric combinations in cosmology of massive bigravity
- A general theory of linear cosmological perturbations: bimetric theories
- On nonlocally interacting metrics, and a simple proposal for cosmic acceleration
- Massive mimetic cosmology
- The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
- Cosmological histories in bimetric gravity: A graphical approach
- Structure Formation in Various Dynamical Dark Energy Scenarios
- Probing alternative cosmologies through the inverse distance ladder
- Cosmology of Massive Gravity and its Extensions
- Aller guten Dinge sind drei: Cosmology with three interacting spin-2 fields
- Perturbations of Cosmological and Black Hole Solutions in Massive gravity and Bi-gravity
- Cosmic variance mitigation in measurements of the integrated Sachs-Wolfe effect