Minimal theory of massive gravity and constraints on the graviton mass
arXiv:2110.01237 · doi:10.1088/1475-7516/2021/12/011
Abstract
The Minimal theory of Massive Gravity (MTMG) is endowed non-linearly with only two tensor modes in the gravity sector which acquire a non-zero mass. On a homogeneous and isotropic background the theory is known to possess two branches: the self-accelerating branch with a phenomenology in cosmology which, except for the mass of the tensor modes, exactly matches the one of CDM; and the normal branch which instead shows deviation from General Relativity in terms of both background and linear perturbations dynamics. For the latter branch we study using several early and late times data sets the constraints on today's value of the graviton mass , finding that at CL, which in turn gives an upper bound at CL as eV. This corresponds to the strongest bound on the mass of the graviton for the normal branch of MTMG.
arXiv comment16 pages, 5 figures, uses revtex
References in corpus (30)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
- The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- Resummation of Massive Gravity
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
- Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code
- Dark Energy after GW170817 and GRB170817A
- Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog
- KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints
- Measurements of the Hubble Constant: Tensions in Perspective
- Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Data Calibration
- A gravitational-wave measurement of the Hubble constant following the second observing run of Advanced LIGO and Virgo
- Graviton Mass Bounds
- Open FRW universes and self-acceleration from nonlinear massive gravity
- Nonlinear stability of cosmological solutions in massive gravity
- Internal Robustness of Growth Rate data
- Minimal theory of massive gravity
- An Updated Tomographic Analysis of the Integrated Sachs-Wolfe Effect and implications for Dark Energy
- Addressing tension by means of VCDM
- Phenomenology in minimal theory of massive gravity
- Signatures of a Graviton Mass in the Cosmic Microwave Background
- Graviton mass might reduce tension between early and late time cosmological data
- Vector disformal transformation of generalized Proca theory
- Cosmological constraints on non-adiabatic dark energy perturbations
- Black holes and stars in the minimal theory of massive gravity
- Integrated Sachs-Wolfe-galaxy cross-correlation bounds on the two branches of the minimal theory of massive gravity
- Baryon Physics and Tight Coupling Approximation in Boltzmann Codes
Cited by in corpus (17)
- VCDM and Cuscuton
- Spin-2 dark matter from anisotropic Universe in bigravity
- Static, spherically symmetric objects in Type-II minimally modified gravity
- Observational bounds on extended minimal theories of massive gravity: New limits on the graviton mass
- Aether-quasi-dilaton massive gravity
- Gravitational collapse and formation of a black hole in a type II minimally modified gravity theory
- Extended minimal theories of massive gravity
- Cosmological Mass of the Photon and Dark Energy as its Bose-Einstein Condensate in de Sitter Space
- Polarization Properties of the Electromagnetic Response to High-frequency Gravitational Wave
- Theory of interacting vector dark energy and fluid
- Static and spherically symmetric general relativity solutions in Minimal Theory of Bigravity
- Generation of effective massive Spin-2 fields through spontaneous symmetry breaking of scalar field
- Gravitational collapse and odd-parity black hole perturbations in Minimal Theory of Bigravity
- The Cosmological Impact of Brane-Chern-Simons Massive Gravity
- Linear growth of structure in massive gravity
- Gravitational ringdown in the Minimal Theory of Massive Gravity
- Spatially covariant gravity with two degrees of freedom in the presence of an auxiliary scalar field: Hamiltonian analysis