Pith. sign in

REVIEW 1 cited by

Cosmological perturbations in Gauss-Bonnet quasi-dilaton massive gravity

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2105.03744 v2 pith:YBF2NQWS submitted 2021-05-08 gr-qc hep-th

classification gr-qchep-th
keywords gauss-bonnetgravitationalgravitymassivequasi-dilatonbackgroundcalculatecosmological
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We present the cosmological analysis of the Gauss-Bonnet quasi-dilaton massive gravity theory. This offers a gravitational theory with a non-zero graviton mass. We calculate the complete set of background equations of motion. Also, we obtain the self-accelerating background solutions and we present the constraints on parameters to indicate the correct sign of parameters. In addition, we analyse tensor perturbations and calculate the mass of graviton and find the dispersion relation of gravitational waves for two cases. Finally, we investigate the propagation of gravitational perturbation in the FLRW cosmology in the Gauss-Bonnet quasi-dilaton massive gravity.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Cosmological horizon thermodynamics in Gauss-Bonnet quasi-dilaton Massive Gravity

    gr-qc 2026-07 reject novelty 5.0 of 10

    Gauss-Bonnet quasi-dilaton massive gravity is claimed to obey horizon thermodynamics and the holographic entropy bound, provided the Gauss-Bonnet coupling is non-negative.

Pith tools