Topological defects in f(T) theory of gravity

Abstract In this paper, we investigate the behaviour of domain walls and one-dimensional cosmic string with locally rotationally symmetric (LRS) Bianchi type-I metric in the context of f(T) gravity. Three different types of deceleration parameter (DP) forms, such as (i) $$q=-kt+l-1$$ q = - k t + l -...

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Main Authors: S. P. Hatkar, D. P. Tadas, S. D. Katore
Format: Article
Language:English
Published: SpringerOpen 2025-02-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-025-13800-2
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author S. P. Hatkar
D. P. Tadas
S. D. Katore
author_facet S. P. Hatkar
D. P. Tadas
S. D. Katore
author_sort S. P. Hatkar
collection DOAJ
description Abstract In this paper, we investigate the behaviour of domain walls and one-dimensional cosmic string with locally rotationally symmetric (LRS) Bianchi type-I metric in the context of f(T) gravity. Three different types of deceleration parameter (DP) forms, such as (i) $$q=-kt+l-1$$ q = - k t + l - 1 , (ii) $$q=b(t)$$ q = b ( t ) , and (iii) $$q=-1+\frac{\gamma }{1+a^\gamma }$$ q = - 1 + γ 1 + a γ , are used to determine the exact solution of the field equation. We observe the profound effect of the torsion scalar T on physical parameters. Also, the universe was dominated by string at an early stage of evaluation.
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institution Kabale University
issn 1434-6052
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series European Physical Journal C: Particles and Fields
spelling doaj-art-bcf97310beef4fa1bf2092cdba12eaa32025-02-09T12:51:36ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522025-02-0185211610.1140/epjc/s10052-025-13800-2Topological defects in f(T) theory of gravityS. P. Hatkar0D. P. Tadas1S. D. Katore2Department of Mathematics, A.E.S. Arts, Commerce and Science CollegeDepartment of Mathematics, Toshniwal Arts, Commerce and Science CollegeDepartment of Mathematics, Sant Gadge Baba Amravati UniversityAbstract In this paper, we investigate the behaviour of domain walls and one-dimensional cosmic string with locally rotationally symmetric (LRS) Bianchi type-I metric in the context of f(T) gravity. Three different types of deceleration parameter (DP) forms, such as (i) $$q=-kt+l-1$$ q = - k t + l - 1 , (ii) $$q=b(t)$$ q = b ( t ) , and (iii) $$q=-1+\frac{\gamma }{1+a^\gamma }$$ q = - 1 + γ 1 + a γ , are used to determine the exact solution of the field equation. We observe the profound effect of the torsion scalar T on physical parameters. Also, the universe was dominated by string at an early stage of evaluation.https://doi.org/10.1140/epjc/s10052-025-13800-2
spellingShingle S. P. Hatkar
D. P. Tadas
S. D. Katore
Topological defects in f(T) theory of gravity
European Physical Journal C: Particles and Fields
title Topological defects in f(T) theory of gravity
title_full Topological defects in f(T) theory of gravity
title_fullStr Topological defects in f(T) theory of gravity
title_full_unstemmed Topological defects in f(T) theory of gravity
title_short Topological defects in f(T) theory of gravity
title_sort topological defects in f t theory of gravity
url https://doi.org/10.1140/epjc/s10052-025-13800-2
work_keys_str_mv AT sphatkar topologicaldefectsinfttheoryofgravity
AT dptadas topologicaldefectsinfttheoryofgravity
AT sdkatore topologicaldefectsinfttheoryofgravity