Generalized Finslerian Wormhole Models in $f(\mathcal{R},\mathcal{T})$ Gravity

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Autori principali: R., Yashwanth B., K., Narasimhamurthy S., Nekouee, Z.
Natura: Preprint
Pubblicazione: 2023
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author R., Yashwanth B.
K., Narasimhamurthy S.
Nekouee, Z.
author_facet R., Yashwanth B.
K., Narasimhamurthy S.
Nekouee, Z.
contents This article explores wormhole solutions within the framework of Finsler geometry and the modified gravity theory. Modifications in gravitational theories, such as $f(\mathcal{R}, \mathcal{T})$ gravity, propose alternatives that potentially avoid the exotic requirements. We derive the field equations to examine the conditions for Finslerian wormhole existence and investigate geometrical and material characteristics of static wormholes using a polynomial shape function in Finslerian space-time. Furthermore, we address energy condition violations for different Finsler parameters graphically. We conclude that the proposed models, which assume a constant redshift function, satisfy the necessary geometric constraints and energy condition violations indicating the presence of exotic matter at the wormhole throat. The results are validated through analytical solutions and 3-D visualizations, contributing to the broader understanding of wormholes in Finsler-modified gravity contexts.
format Preprint
id arxiv_https___arxiv_org_abs_2302_09788
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Generalized Finslerian Wormhole Models in $f(\mathcal{R},\mathcal{T})$ Gravity
R., Yashwanth B.
K., Narasimhamurthy S.
Nekouee, Z.
General Relativity and Quantum Cosmology
83C10, 53C60, 83-10, 53Z05
This article explores wormhole solutions within the framework of Finsler geometry and the modified gravity theory. Modifications in gravitational theories, such as $f(\mathcal{R}, \mathcal{T})$ gravity, propose alternatives that potentially avoid the exotic requirements. We derive the field equations to examine the conditions for Finslerian wormhole existence and investigate geometrical and material characteristics of static wormholes using a polynomial shape function in Finslerian space-time. Furthermore, we address energy condition violations for different Finsler parameters graphically. We conclude that the proposed models, which assume a constant redshift function, satisfy the necessary geometric constraints and energy condition violations indicating the presence of exotic matter at the wormhole throat. The results are validated through analytical solutions and 3-D visualizations, contributing to the broader understanding of wormholes in Finsler-modified gravity contexts.
title Generalized Finslerian Wormhole Models in $f(\mathcal{R},\mathcal{T})$ Gravity
topic General Relativity and Quantum Cosmology
83C10, 53C60, 83-10, 53Z05
url https://arxiv.org/abs/2302.09788