Compact star in noninteger power model of $f(R)$ gravity

Fuente: arXiv
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Autori principali: Cui, Yong-Xiang, Yan, Zu, Numajiri, Kota, Katsuragawa, Taishi, Nojiri, Shin'ichi
Natura: Preprint
Pubblicazione: 2024
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author Cui, Yong-Xiang
Yan, Zu
Numajiri, Kota
Katsuragawa, Taishi
Nojiri, Shin'ichi
author_facet Cui, Yong-Xiang
Yan, Zu
Numajiri, Kota
Katsuragawa, Taishi
Nojiri, Shin'ichi
contents We investigate compact stars in the noninteger power (NIP) model of $f(R)$ gravity theory, which includes the higher-curvature correction to the Einstein-Hilbert action. The mass-radius relation of the compact stars in the NIP model predicts large deviations from those in the general relativity in the low-mass region, potentially allowing us to test the NIP model by future astrophysical observations. We also study the nonvanishing scalar hair surrounding the compact star and demonstrate that the chameleon mechanism works efficiently. They result in distinct scalar profiles inside and outside the star, which implies screening the fifth force mediated by the scalar field.
format Preprint
id arxiv_https___arxiv_org_abs_2408_12301
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Compact star in noninteger power model of $f(R)$ gravity
Cui, Yong-Xiang
Yan, Zu
Numajiri, Kota
Katsuragawa, Taishi
Nojiri, Shin'ichi
General Relativity and Quantum Cosmology
High Energy Physics - Theory
We investigate compact stars in the noninteger power (NIP) model of $f(R)$ gravity theory, which includes the higher-curvature correction to the Einstein-Hilbert action. The mass-radius relation of the compact stars in the NIP model predicts large deviations from those in the general relativity in the low-mass region, potentially allowing us to test the NIP model by future astrophysical observations. We also study the nonvanishing scalar hair surrounding the compact star and demonstrate that the chameleon mechanism works efficiently. They result in distinct scalar profiles inside and outside the star, which implies screening the fifth force mediated by the scalar field.
title Compact star in noninteger power model of $f(R)$ gravity
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2408.12301