Wormholes in the f(R,L,T) theory of gravity

Fuente: arXiv
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Main Authors: Moraes, P. H. R. S., Agrawal, A. S., Mishra, B.
Format: Preprint
Published: 2024
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author Moraes, P. H. R. S.
Agrawal, A. S.
Mishra, B.
author_facet Moraes, P. H. R. S.
Agrawal, A. S.
Mishra, B.
contents Morris and Thorne developed wormhole solutions in the late 1980s when they discovered a recipe that wormholes must follow for travelers to cross them safely. They describe exotic matter as satisfying $-p_{r} > ρ$, where $p_{r}$ is the radial pressure and $ρ$ is the energy density of the wormhole. This is a notable characteristic of the General Relativity Theory. The current article discusses traversable wormhole solutions in $f(R, L, T)=R+αL+βT$, with $α$ and $β$ are model parameters. The wormhole solutions presented here satisfy the metric constraints of traversability while remarkably avoiding the exotic matter condition, indicating that $f(R, L, T)$ gravity wormholes can be filled with ordinary matter. The derived solutions for the shape function of the wormhole meet the required metric conditions. They exhibit behavior that is comparable to that of wormholes reported in earlier references, which is also the case for our solutions for the energy density of such objects.
format Preprint
id arxiv_https___arxiv_org_abs_2403_00310
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Wormholes in the f(R,L,T) theory of gravity
Moraes, P. H. R. S.
Agrawal, A. S.
Mishra, B.
General Relativity and Quantum Cosmology
Morris and Thorne developed wormhole solutions in the late 1980s when they discovered a recipe that wormholes must follow for travelers to cross them safely. They describe exotic matter as satisfying $-p_{r} > ρ$, where $p_{r}$ is the radial pressure and $ρ$ is the energy density of the wormhole. This is a notable characteristic of the General Relativity Theory. The current article discusses traversable wormhole solutions in $f(R, L, T)=R+αL+βT$, with $α$ and $β$ are model parameters. The wormhole solutions presented here satisfy the metric constraints of traversability while remarkably avoiding the exotic matter condition, indicating that $f(R, L, T)$ gravity wormholes can be filled with ordinary matter. The derived solutions for the shape function of the wormhole meet the required metric conditions. They exhibit behavior that is comparable to that of wormholes reported in earlier references, which is also the case for our solutions for the energy density of such objects.
title Wormholes in the f(R,L,T) theory of gravity
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2403.00310