Graviton mass might reduce tension between early and late time cosmological data
Antonio De Felice, Shinji Mukohyama

TL;DR
This paper proposes that a small non-zero graviton mass within the Minimal Theory of Massive Gravity can reconcile discrepancies between early universe and late-time cosmological data, improving model fit and constraining graviton mass.
Contribution
It introduces a modified gravity model where graviton mass affects matter perturbations without altering background evolution, addressing tensions in cosmological measurements.
Findings
MTMG fits RSD data better than $$-CDM by two orders of magnitude.
The graviton mass squared is constrained to about b1 (3d7 10^{-33} eV)^2.
The graviton mass estimate is consistent with LIGO bounds.
Abstract
The standard -CDM predicts a growth of structures which tends to be higher than the values of redshift space distortion (RSD) measurements, if the cosmological parameters are fixed by the CMB data. In this paper we point out that this discrepancy can be resolved/understood if we assume that the graviton has a small but non-zero mass. In the context of the Minimal Theory of Massive Gravity (MTMG), due to infrared Lorentz violations measurable only at present cosmological scales, the graviton acquires a mass without being haunted by unwanted extra degrees of freedom. While the so-called self-accelerating branch of cosmological solutions in MTMG has the same phenomenology for the background as well as the scalar- and vector-type linear perturbations as the -CDM in General Relativity (GR), it is possible to choose another branch so that the background is the same as that…
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