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Bibliographic Details
Main Authors: Campbell, Mariam, Carloni, Sante, Dunsby, Peter K. S., Naidu, Nolene F.
Format: Preprint
Published: 2024
Subjects:
Online Access:https://arxiv.org/abs/2403.00070
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author Campbell, Mariam
Carloni, Sante
Dunsby, Peter K. S.
Naidu, Nolene F.
author_facet Campbell, Mariam
Carloni, Sante
Dunsby, Peter K. S.
Naidu, Nolene F.
contents We present a covariant description of non-vacuum static spherically symmetric spacetimes in $f(R)$ gravity applying the (1+1+2) covariant formalism. The propagation equations are then used to derive a covariant and dimensionless form of the Tolman-Oppenheimer-Volkoff (TOV) equations. We then give a solution strategy to these equations and obtain some new exact solutions for the particular case $f(R)=R+αR^{2}$, which have the correct thermodynamic properties for standard matter.
format Preprint
id arxiv_https___arxiv_org_abs_2403_00070
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Some exact relativistic star solutions in $f(R)$ gravity
Campbell, Mariam
Carloni, Sante
Dunsby, Peter K. S.
Naidu, Nolene F.
General Relativity and Quantum Cosmology
High Energy Physics - Theory
We present a covariant description of non-vacuum static spherically symmetric spacetimes in $f(R)$ gravity applying the (1+1+2) covariant formalism. The propagation equations are then used to derive a covariant and dimensionless form of the Tolman-Oppenheimer-Volkoff (TOV) equations. We then give a solution strategy to these equations and obtain some new exact solutions for the particular case $f(R)=R+αR^{2}$, which have the correct thermodynamic properties for standard matter.
title Some exact relativistic star solutions in $f(R)$ gravity
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2403.00070