Domain Wall Bianchi Type VI0 Universe in f(R, T) Gravity

IF 0.7 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Astrophysics Pub Date : 2025-01-17 DOI:10.1007/s10511-025-09850-9
S. P. Hatkar, D. P. Tadas, S. D. Katore
{"title":"Domain Wall Bianchi Type VI0 Universe in f(R, T) Gravity","authors":"S. P. Hatkar,&nbsp;D. P. Tadas,&nbsp;S. D. Katore","doi":"10.1007/s10511-025-09850-9","DOIUrl":null,"url":null,"abstract":"<p>We consider the Bianchi type-VI<sub>0</sub> space time with domain walls in the framework of the modified f (R, T) theory of gravitation. To solve the field equations, we assume that the shear scalar σ is proportional to the expansion scalar θ. We also consider the parametrization of the equation of the state parameter of barotropic fluid and discuss the effect on domain walls. It has been observed that the domain wall may behave like dark energy. Some physical parameters are also discussed in detail.</p>","PeriodicalId":479,"journal":{"name":"Astrophysics","volume":"67 4","pages":"537 - 555"},"PeriodicalIF":0.7000,"publicationDate":"2025-01-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astrophysics","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s10511-025-09850-9","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

Abstract

We consider the Bianchi type-VI0 space time with domain walls in the framework of the modified f (R, T) theory of gravitation. To solve the field equations, we assume that the shear scalar σ is proportional to the expansion scalar θ. We also consider the parametrization of the equation of the state parameter of barotropic fluid and discuss the effect on domain walls. It has been observed that the domain wall may behave like dark energy. Some physical parameters are also discussed in detail.

查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
域壁Bianchi型VI0宇宙在f(R, T)引力
我们在修正的f (R, T)引力理论的框架下考虑带畴壁的Bianchi - vi0型时空。为了求解场方程,我们假设剪切标量σ与膨胀标量θ成正比。本文还考虑了正压流体状态参数方程的参数化,并讨论了其对畴壁的影响。已经观察到,畴壁可能表现得像暗能量。对一些物理参数也进行了详细的讨论。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 去求助
来源期刊
Astrophysics
Astrophysics 地学天文-天文与天体物理
CiteScore
0.90
自引率
20.00%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Astrophysics (Ap) is a peer-reviewed scientific journal which publishes research in theoretical and observational astrophysics. Founded by V.A.Ambartsumian in 1965 Astrophysics is one of the international astronomy journals. The journal covers space astrophysics, stellar and galactic evolution, solar physics, stellar and planetary atmospheres, interstellar matter. Additional subjects include chemical composition and internal structure of stars, quasars and pulsars, developments in modern cosmology and radiative transfer.
期刊最新文献
The Smooth Bounce: How Anisotropy and f(R,T) Gravity Preserve Perturbations in a Bianchi-V Cosmology Review of Recent Findings on Chemical Composition of Red Giants with Magnetic Fields On Galactic Distribution of Different Pulsars Temperature Effects in the Proto Neutron Star Phase of PSR J0740+6620 A Novel Parametrized Dark Energy Model in a Flat Universe
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1