Scalar induced gravitational waves in f(R) gravity

Fuente: arXiv
Salvato in:
Dettagli Bibliografici
Autori principali: Zhou, Jing-Zhi, Kuang, Yu-Ting, Wu, Di, Chen, Fei-Yu, Lü, H., Chang, Zhe
Natura: Preprint
Pubblicazione: 2024
Soggetti:
Accesso online:
Tags: Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
_version_ 1866913577083863040
author Zhou, Jing-Zhi
Kuang, Yu-Ting
Wu, Di
Chen, Fei-Yu
Lü, H.
Chang, Zhe
author_facet Zhou, Jing-Zhi
Kuang, Yu-Ting
Wu, Di
Chen, Fei-Yu
Lü, H.
Chang, Zhe
contents We investigate the first and second order cosmological perturbation equations in f(R) modified gravity theory and provide the equation of motion of second order scalar induced gravitational waves. We find that the effects of modified gravity not only change the form of the equation of motion of second order scalar induced gravitational waves but also contribute an additional anisotropic stress tensor, composed of first order scalar perturbations, to the source term of the gravitational waves. We calculate the energy density spectrum of second order scalar induced gravitational waves in the HS model. Utilizing current pulsar timing array observational data, we perform a rigorous Bayesian analysis of the parameter space of the HS model.
format Preprint
id arxiv_https___arxiv_org_abs_2409_07702
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Scalar induced gravitational waves in f(R) gravity
Zhou, Jing-Zhi
Kuang, Yu-Ting
Wu, Di
Chen, Fei-Yu
Lü, H.
Chang, Zhe
General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Theory
We investigate the first and second order cosmological perturbation equations in f(R) modified gravity theory and provide the equation of motion of second order scalar induced gravitational waves. We find that the effects of modified gravity not only change the form of the equation of motion of second order scalar induced gravitational waves but also contribute an additional anisotropic stress tensor, composed of first order scalar perturbations, to the source term of the gravitational waves. We calculate the energy density spectrum of second order scalar induced gravitational waves in the HS model. Utilizing current pulsar timing array observational data, we perform a rigorous Bayesian analysis of the parameter space of the HS model.
title Scalar induced gravitational waves in f(R) gravity
topic General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Theory
url https://arxiv.org/abs/2409.07702