二次f ( Q ) $f(Q)$引力中以五弦场为特征的无奇点恒星模型

IF 5.6 3区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY
Piyali Bhar
{"title":"二次f ( Q ) $f(Q)$引力中以五弦场为特征的无奇点恒星模型","authors":"Piyali Bhar","doi":"10.1002/prop.202300183","DOIUrl":null,"url":null,"abstract":"<p>In the context of the <math>\n <semantics>\n <mrow>\n <mi>f</mi>\n <mo>(</mo>\n <mi>Q</mi>\n <mo>)</mo>\n </mrow>\n <annotation>$f(Q)$</annotation>\n </semantics></math> theory of gravity, a spherically symmetric quintessence DE model in this article is offered. For this reason, <math>\n <semantics>\n <mrow>\n <mi>f</mi>\n <mo>(</mo>\n <mi>Q</mi>\n <mo>)</mo>\n </mrow>\n <annotation>$f(Q)$</annotation>\n </semantics></math> has the formula <math>\n <semantics>\n <mrow>\n <mi>f</mi>\n <mrow>\n <mo>(</mo>\n <mi>Q</mi>\n <mo>)</mo>\n </mrow>\n <mo>=</mo>\n <mi>a</mi>\n <msup>\n <mi>Q</mi>\n <mn>2</mn>\n </msup>\n <mo>+</mo>\n <mi>Q</mi>\n </mrow>\n <annotation>$f(Q)=aQ^2+Q$</annotation>\n </semantics></math>, where <i>Q</i> stands for the non-metricity scalar and ‘a’ is the coupling constant for modified gravity has been taken into account. It is supposed that the quintessence field defined by the parameter <math>\n <semantics>\n <msub>\n <mi>ω</mi>\n <mi>q</mi>\n </msub>\n <annotation>$\\omega _q$</annotation>\n </semantics></math>, where <math>\n <semantics>\n <mrow>\n <msub>\n <mi>ω</mi>\n <mi>q</mi>\n </msub>\n <mo>∈</mo>\n <mrow>\n <mo>(</mo>\n <mo>−</mo>\n <mn>1</mn>\n <mo>,</mo>\n <mspace></mspace>\n <mo>−</mo>\n <mfrac>\n <mn>1</mn>\n <mn>3</mn>\n </mfrac>\n <mo>)</mo>\n </mrow>\n </mrow>\n <annotation>$\\omega _q \\in (-1,\\,-\\frac{1}{3})$</annotation>\n </semantics></math>, controls the energy-momentum tensor of the underlying fluid distribution. The relationship between several physical parameters for the selected values of ‘a’, by choosing the metric potentials suggested by the Krori-Barua [Krori and Barua; <i>J. Phys. A, Math. Gen</i>. <b>8</b>: 508, 1975] is investigated. Further, a number of analyses in detail to examine the physical validity of the proposed stellar model are carried out. The consequences of the compact star system caused by the connection of matter and geometry are succinctly described. The maximum allowable mass and radius for our present model for different values of ‘a’ have been studied by <math>\n <semantics>\n <mrow>\n <mi>M</mi>\n <mo>−</mo>\n <mi>R</mi>\n </mrow>\n <annotation>$M-R$</annotation>\n </semantics></math> and <math>\n <semantics>\n <mrow>\n <mi>M</mi>\n <mo>−</mo>\n <msub>\n <mi>ρ</mi>\n <mi>c</mi>\n </msub>\n </mrow>\n <annotation>$M-\\rho _c$</annotation>\n </semantics></math> curve. One can recover the usual general relativity (GR) standard results for <math>\n <semantics>\n <mrow>\n <mi>a</mi>\n <mo>=</mo>\n <mn>0</mn>\n </mrow>\n <annotation>$a=0$</annotation>\n </semantics></math>.</p>","PeriodicalId":55150,"journal":{"name":"Fortschritte Der Physik-Progress of Physics","volume":"72 1","pages":""},"PeriodicalIF":5.6000,"publicationDate":"2023-10-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Singularity Free Star Model Characterized by Quintessence Field in Quadratic \\n \\n \\n f\\n (\\n Q\\n )\\n \\n $f(Q)$\\n Gravity\",\"authors\":\"Piyali Bhar\",\"doi\":\"10.1002/prop.202300183\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>In the context of the <math>\\n <semantics>\\n <mrow>\\n <mi>f</mi>\\n <mo>(</mo>\\n <mi>Q</mi>\\n <mo>)</mo>\\n </mrow>\\n <annotation>$f(Q)$</annotation>\\n </semantics></math> theory of gravity, a spherically symmetric quintessence DE model in this article is offered. For this reason, <math>\\n <semantics>\\n <mrow>\\n <mi>f</mi>\\n <mo>(</mo>\\n <mi>Q</mi>\\n <mo>)</mo>\\n </mrow>\\n <annotation>$f(Q)$</annotation>\\n </semantics></math> has the formula <math>\\n <semantics>\\n <mrow>\\n <mi>f</mi>\\n <mrow>\\n <mo>(</mo>\\n <mi>Q</mi>\\n <mo>)</mo>\\n </mrow>\\n <mo>=</mo>\\n <mi>a</mi>\\n <msup>\\n <mi>Q</mi>\\n <mn>2</mn>\\n </msup>\\n <mo>+</mo>\\n <mi>Q</mi>\\n </mrow>\\n <annotation>$f(Q)=aQ^2+Q$</annotation>\\n </semantics></math>, where <i>Q</i> stands for the non-metricity scalar and ‘a’ is the coupling constant for modified gravity has been taken into account. It is supposed that the quintessence field defined by the parameter <math>\\n <semantics>\\n <msub>\\n <mi>ω</mi>\\n <mi>q</mi>\\n </msub>\\n <annotation>$\\\\omega _q$</annotation>\\n </semantics></math>, where <math>\\n <semantics>\\n <mrow>\\n <msub>\\n <mi>ω</mi>\\n <mi>q</mi>\\n </msub>\\n <mo>∈</mo>\\n <mrow>\\n <mo>(</mo>\\n <mo>−</mo>\\n <mn>1</mn>\\n <mo>,</mo>\\n <mspace></mspace>\\n <mo>−</mo>\\n <mfrac>\\n <mn>1</mn>\\n <mn>3</mn>\\n </mfrac>\\n <mo>)</mo>\\n </mrow>\\n </mrow>\\n <annotation>$\\\\omega _q \\\\in (-1,\\\\,-\\\\frac{1}{3})$</annotation>\\n </semantics></math>, controls the energy-momentum tensor of the underlying fluid distribution. The relationship between several physical parameters for the selected values of ‘a’, by choosing the metric potentials suggested by the Krori-Barua [Krori and Barua; <i>J. Phys. A, Math. Gen</i>. <b>8</b>: 508, 1975] is investigated. Further, a number of analyses in detail to examine the physical validity of the proposed stellar model are carried out. The consequences of the compact star system caused by the connection of matter and geometry are succinctly described. The maximum allowable mass and radius for our present model for different values of ‘a’ have been studied by <math>\\n <semantics>\\n <mrow>\\n <mi>M</mi>\\n <mo>−</mo>\\n <mi>R</mi>\\n </mrow>\\n <annotation>$M-R$</annotation>\\n </semantics></math> and <math>\\n <semantics>\\n <mrow>\\n <mi>M</mi>\\n <mo>−</mo>\\n <msub>\\n <mi>ρ</mi>\\n <mi>c</mi>\\n </msub>\\n </mrow>\\n <annotation>$M-\\\\rho _c$</annotation>\\n </semantics></math> curve. One can recover the usual general relativity (GR) standard results for <math>\\n <semantics>\\n <mrow>\\n <mi>a</mi>\\n <mo>=</mo>\\n <mn>0</mn>\\n </mrow>\\n <annotation>$a=0$</annotation>\\n </semantics></math>.</p>\",\"PeriodicalId\":55150,\"journal\":{\"name\":\"Fortschritte Der Physik-Progress of Physics\",\"volume\":\"72 1\",\"pages\":\"\"},\"PeriodicalIF\":5.6000,\"publicationDate\":\"2023-10-26\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Fortschritte Der Physik-Progress of Physics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://onlinelibrary.wiley.com/doi/10.1002/prop.202300183\",\"RegionNum\":3,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"PHYSICS, MULTIDISCIPLINARY\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Fortschritte Der Physik-Progress of Physics","FirstCategoryId":"101","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1002/prop.202300183","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0

摘要

在 f ( Q ) $f(Q)$引力理论的背景下,本文提出了一个球对称五重 DE 模型。因此,f ( Q ) $f(Q)$ 的公式为 f ( Q ) = a Q 2 + Q $f(Q)=aQ^2+Q$ ,其中 Q 代表非度量标量,'a'为修正引力的耦合常数。假定由参数 ω q $\omega _q$ 定义的五元场,其中 ω q ∈ ( - 1 , - 1 3 ) $\omega _q \ in (-1,\,-\frac{1}{3})$ 控制底层流体分布的能量-动量张量。通过选择 Krori-Barua [Krori and Barua; J. Phys. A, Math. Gen. 8: 508, 1975] 提出的度量势,研究了'a'的选定值与几个物理参数之间的关系。此外,还进行了一系列详细分析,以检验所提出的恒星模型的物理有效性。简明扼要地描述了物质和几何之间的联系所导致的紧凑恒星系统的后果。我们用 M - R $M-R$ 和 M - ρ c $M-\rho _c$ 曲线研究了不同'a'值下我们目前模型的最大允许质量和半径。在 a = 0 $a=0$ 的情况下,我们可以得到通常的广义相对论(GR)标准结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Singularity Free Star Model Characterized by Quintessence Field in Quadratic f ( Q ) $f(Q)$ Gravity

In the context of the f ( Q ) $f(Q)$ theory of gravity, a spherically symmetric quintessence DE model in this article is offered. For this reason, f ( Q ) $f(Q)$ has the formula f ( Q ) = a Q 2 + Q $f(Q)=aQ^2+Q$ , where Q stands for the non-metricity scalar and ‘a’ is the coupling constant for modified gravity has been taken into account. It is supposed that the quintessence field defined by the parameter ω q $\omega _q$ , where ω q ( 1 , 1 3 ) $\omega _q \in (-1,\,-\frac{1}{3})$ , controls the energy-momentum tensor of the underlying fluid distribution. The relationship between several physical parameters for the selected values of ‘a’, by choosing the metric potentials suggested by the Krori-Barua [Krori and Barua; J. Phys. A, Math. Gen. 8: 508, 1975] is investigated. Further, a number of analyses in detail to examine the physical validity of the proposed stellar model are carried out. The consequences of the compact star system caused by the connection of matter and geometry are succinctly described. The maximum allowable mass and radius for our present model for different values of ‘a’ have been studied by M R $M-R$ and M ρ c $M-\rho _c$ curve. One can recover the usual general relativity (GR) standard results for a = 0 $a=0$ .

求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
CiteScore
6.70
自引率
7.70%
发文量
75
审稿时长
6-12 weeks
期刊介绍: The journal Fortschritte der Physik - Progress of Physics is a pure online Journal (since 2013). Fortschritte der Physik - Progress of Physics is devoted to the theoretical and experimental studies of fundamental constituents of matter and their interactions e. g. elementary particle physics, classical and quantum field theory, the theory of gravitation and cosmology, quantum information, thermodynamics and statistics, laser physics and nonlinear dynamics, including chaos and quantum chaos. Generally the papers are review articles with a detailed survey on relevant publications, but original papers of general interest are also published.
×
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
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
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 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信