Gauge invariant perturbations in teleparallel Horndeski gravity

Fuente: arXiv
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Hauptverfasser: Ahmedov, Bobomurat, Caruana, Maria, Said, Jackson Levi, Dialektopoulos, Konstantinos F., Nosirov, Abdurakhmon, Oikonomopoulou, Zinovia, Yunusov, Odil
Format: Preprint
Veröffentlicht: 2024
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author Ahmedov, Bobomurat
Caruana, Maria
Said, Jackson Levi
Dialektopoulos, Konstantinos F.
Nosirov, Abdurakhmon
Oikonomopoulou, Zinovia
Yunusov, Odil
author_facet Ahmedov, Bobomurat
Caruana, Maria
Said, Jackson Levi
Dialektopoulos, Konstantinos F.
Nosirov, Abdurakhmon
Oikonomopoulou, Zinovia
Yunusov, Odil
contents We present in the form of a catalogue of the cosmological perturbations within the Bahamonde- Dialektopoulos-Levi Said (BDLS) theory, which serves as the teleparallel counterpart of Horndeski gravity. To understand structure formation in cosmological models, it is essential to study both the background and perturbative aspects of their cosmology. While extensive analysis of both Horndeski gravity and its teleparallel analog exists in the literature, a quantitative understanding requires a detailed examination of their cosmological perturbations. We review here all the different gauges for the scalar, vector and tensor perturbations of a cosmological background up to second order and we hope this will help people who work with observations, to incorporate it in existing codes.
format Preprint
id arxiv_https___arxiv_org_abs_2412_01349
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Gauge invariant perturbations in teleparallel Horndeski gravity
Ahmedov, Bobomurat
Caruana, Maria
Said, Jackson Levi
Dialektopoulos, Konstantinos F.
Nosirov, Abdurakhmon
Oikonomopoulou, Zinovia
Yunusov, Odil
General Relativity and Quantum Cosmology
We present in the form of a catalogue of the cosmological perturbations within the Bahamonde- Dialektopoulos-Levi Said (BDLS) theory, which serves as the teleparallel counterpart of Horndeski gravity. To understand structure formation in cosmological models, it is essential to study both the background and perturbative aspects of their cosmology. While extensive analysis of both Horndeski gravity and its teleparallel analog exists in the literature, a quantitative understanding requires a detailed examination of their cosmological perturbations. We review here all the different gauges for the scalar, vector and tensor perturbations of a cosmological background up to second order and we hope this will help people who work with observations, to incorporate it in existing codes.
title Gauge invariant perturbations in teleparallel Horndeski gravity
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2412.01349