A new solution of Einstein’s field equations in isotropic coordinates

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Journal of Astrophysics and Astronomy Pub Date : 2024-06-13 DOI:10.1007/s12036-024-10006-y
B. S. Ratanpal, BHAVESH Suthar
{"title":"A new solution of Einstein’s field equations in isotropic coordinates","authors":"B. S. Ratanpal,&nbsp;BHAVESH Suthar","doi":"10.1007/s12036-024-10006-y","DOIUrl":null,"url":null,"abstract":"<div><p>In this work, an exact solution of Einstein’s field equations in isotropic coordinates for anisotropic matter distribution is obtained by considering a particular metric choice of metric potential <span>\\(g_{rr}\\)</span>. To check the feasibility of the model, we have investigated all the physical characteristics of a realistic star. It is found that the model is potentially stable, and the adiabatic index is greater than <span>\\(\\frac{4}{3}\\)</span>. The model has been analyzed for compact star 4U 1538-52.</p></div>","PeriodicalId":610,"journal":{"name":"Journal of Astrophysics and Astronomy","volume":"45 2","pages":""},"PeriodicalIF":1.1000,"publicationDate":"2024-06-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Astrophysics and Astronomy","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s12036-024-10006-y","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

Abstract

In this work, an exact solution of Einstein’s field equations in isotropic coordinates for anisotropic matter distribution is obtained by considering a particular metric choice of metric potential \(g_{rr}\). To check the feasibility of the model, we have investigated all the physical characteristics of a realistic star. It is found that the model is potentially stable, and the adiabatic index is greater than \(\frac{4}{3}\). The model has been analyzed for compact star 4U 1538-52.

Abstract Image

Abstract Image

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
各向同性坐标下爱因斯坦场方程的新解
在这项工作中,通过考虑特定度量选择的度量势 \(g_{rr}\),得到了各向异性物质分布的各向同性坐标下爱因斯坦场方程的精确解。为了检验模型的可行性,我们研究了现实恒星的所有物理特征。结果发现该模型是潜在稳定的,绝热指数大于 \(\frac{4}{3}\)。该模型针对紧凑恒星 4U 1538-52 进行了分析。
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
Journal of Astrophysics and Astronomy
Journal of Astrophysics and Astronomy 地学天文-天文与天体物理
CiteScore
1.80
自引率
9.10%
发文量
84
审稿时长
>12 weeks
期刊介绍: The journal publishes original research papers on all aspects of astrophysics and astronomy, including instrumentation, laboratory astrophysics, and cosmology. Critical reviews of topical fields are also published. Articles submitted as letters will be considered.
期刊最新文献
Detection of X-ray polarization in the high synchrotron peaked blazar 1ES 1959\(+\)650 A summary of instruments proposed for observing pulsating variables from the Mt. Abu Observatory Effect of gravitational stratification, longitudinal temperature inhomogeneity, radiative cooling and background plasma flow on torsional Alfvén oscillations of a coronal loop Most powerful maser in the Galaxy is source G25.65+1.05 and the most powerful emitter in the Universe AGN S 0528+134 ALMA detection of hydrogen cyanide in the atmosphere of Saturn
×
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:481959085
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