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ASTROPHYSICS AND COSMOLOGY
Perturbations in Horndeski theory above anisotropic cosmological background
S. A. Mironovabc, A. M. Shtennikovada a Institute for Nuclear Research, Russian Academy of Sciences, Moscow, 117312 Russia
b Institute for Theoretical and Mathematical Physics, Moscow State University, Moscow, 119991 Russia
c National Research Center Kurchatov Institute, Moscow, 123182 Russia
d Department of Particle Physics and Cosmology, Faculty of Physics, Moscow State University, Moscow, 119991 Russia
Abstract:
Considering an anisotropic cosmological background is an interesting and simultaneously challenging problem of theoretical physics, since we not only assume a high degree of anisotropy in the early stages of the Universe, but also observe it to a small degree until now. In this paper we have constructed the unconstrained action for the perturbations above Bianchi I type background in the most general scalar-tensor theory of gravity, the Horndeski theory, and evaluate the effect of the deviation from the anisotropic background on the previously established stable solution obtained in previous works.
Received: 01.07.2023 Revised: 27.01.2024 Accepted: 28.01.2024
Citation:
S. A. Mironov, A. M. Shtennikova, “Perturbations in Horndeski theory above anisotropic cosmological background”, Pis'ma v Zh. Èksper. Teoret. Fiz., 119:5 (2024), 330–335; JETP Letters, 119:5 (2024), 339–344
Linking options:
https://www.mathnet.ru/eng/jetpl7167 https://www.mathnet.ru/eng/jetpl/v119/i5/p330
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