Cosmology in Brans–Dicke–de Rham–Gabadadze–Tolley massive gravity

Sobhan Kazempour and Amin Rezaei Akbarieh
Phys. Rev. D 105, 123515 – Published 15 June 2022

Abstract

We introduce the Brans–Dick–de Rham–Gabadadze–Tolley massive gravity theory which is the new extension of nonlinear massive gravity. We demonstrate a detailed study of the cosmological properties of this theory of gravity, and we show the transformation of the Jordan frame to the Einstein frame. We obtain the cosmological background equations and show the analyses of self-accelerating solutions for explaining the accelerated expansion of the Universe. In the following, we analyze the background perturbations, which consist of tensor, vector, and scalar perturbations within the framework of the new extension of the de Rham–Gabadadze–Tolley massive gravity in the Friedman-Lemaître-Robertson-Walker cosmology.

  • Figure
  • Received 13 April 2022
  • Accepted 7 June 2022

DOI:https://doi.org/10.1103/PhysRevD.105.123515

© 2022 American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Sobhan Kazempour* and Amin Rezaei Akbarieh

  • Faculty of Physics, University of Tabriz, Tabriz 51666-16471, Iran

  • *s.kazempour@tabrizu.ac.ir
  • am.rezaei@tabrizu.ac.ir

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Issue

Vol. 105, Iss. 12 — 15 June 2022

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