动态AdS黑洞的受限相空间热力学:不同熵模型的比较分析

IF 2.1 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Abhishek Baruah, Prabwal Phukon
{"title":"动态AdS黑洞的受限相空间热力学:不同熵模型的比较分析","authors":"Abhishek Baruah,&nbsp;Prabwal Phukon","doi":"10.1007/s10714-025-03413-1","DOIUrl":null,"url":null,"abstract":"<div><p>Using the restricted phase space (RPST) formalism, we perform a comparative study of 4D dyonic AdS black hole thermodynamics in Gibbs–Boltzmann statistics and Rényi statistics. In RPST formalism, instead of pressure and volume, one considers central charge <i>C</i> and chemical potential <span>\\(\\mu \\)</span> as thermodynamic variables. Inclusion of the magnetic charge <span>\\(\\tilde{Q}_m\\)</span> gives rise to a richer phase structure of the study of thermodynamics by adding a non-equilibrium transition from an unstable small black hole to a stable black hole in the <i>T</i>–<i>S</i> processes and a Hawking–Page and Davies type phase transition in the <i>F</i>–<i>T</i> and specific heat plots on top of the Van der Waals and superfluid <span>\\(\\lambda \\)</span> phase transitions. We study an extra mixed ensemble (<span>\\(\\tilde{\\Phi }_e,\\tilde{Q}_m)\\)</span> due to the inclusion of <span>\\(\\tilde{Q}_m\\)</span> where we see Van der Waals phase transition and whose plots change as the entropy model changes meaning for isovoltage processes we see Hawking–Page transition in Bekenstein–Hawking entropy and absence of Hawking–Page in Rényi entropy construct. We observe an interesting phenomenon where changing the Rényi parameter <span>\\(\\lambda \\)</span>, the <i>T</i>–<i>S</i> process changes the same way as when varying the central charge <i>C</i> underlining some similarity that is not seen in the Bekenstein Hawking entropy model. We observe a similarity between the plots when both charges are turned off relating to the Schwarzschild black hole and the grand-canonical ensemble. One can observe that as the entropy models are changed, the homogeneity is not lost where the mass as a function of extensive variables is of order one and the rest zero. We see a similarity in the <span>\\(\\mu \\)</span>–<i>C</i> process across the entropy models signally some universality across entropy models as well as different types of black holes studied before. Finally, we do not see a new universality class for modified entropy as it is seen in studies done for alternate gravity models.\n</p></div>","PeriodicalId":578,"journal":{"name":"General Relativity and Gravitation","volume":"57 5","pages":""},"PeriodicalIF":2.1000,"publicationDate":"2025-05-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Restricted phase space thermodynamics of dyonic AdS black holes: comparative analysis using different entropy models\",\"authors\":\"Abhishek Baruah,&nbsp;Prabwal Phukon\",\"doi\":\"10.1007/s10714-025-03413-1\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>Using the restricted phase space (RPST) formalism, we perform a comparative study of 4D dyonic AdS black hole thermodynamics in Gibbs–Boltzmann statistics and Rényi statistics. In RPST formalism, instead of pressure and volume, one considers central charge <i>C</i> and chemical potential <span>\\\\(\\\\mu \\\\)</span> as thermodynamic variables. Inclusion of the magnetic charge <span>\\\\(\\\\tilde{Q}_m\\\\)</span> gives rise to a richer phase structure of the study of thermodynamics by adding a non-equilibrium transition from an unstable small black hole to a stable black hole in the <i>T</i>–<i>S</i> processes and a Hawking–Page and Davies type phase transition in the <i>F</i>–<i>T</i> and specific heat plots on top of the Van der Waals and superfluid <span>\\\\(\\\\lambda \\\\)</span> phase transitions. We study an extra mixed ensemble (<span>\\\\(\\\\tilde{\\\\Phi }_e,\\\\tilde{Q}_m)\\\\)</span> due to the inclusion of <span>\\\\(\\\\tilde{Q}_m\\\\)</span> where we see Van der Waals phase transition and whose plots change as the entropy model changes meaning for isovoltage processes we see Hawking–Page transition in Bekenstein–Hawking entropy and absence of Hawking–Page in Rényi entropy construct. We observe an interesting phenomenon where changing the Rényi parameter <span>\\\\(\\\\lambda \\\\)</span>, the <i>T</i>–<i>S</i> process changes the same way as when varying the central charge <i>C</i> underlining some similarity that is not seen in the Bekenstein Hawking entropy model. We observe a similarity between the plots when both charges are turned off relating to the Schwarzschild black hole and the grand-canonical ensemble. One can observe that as the entropy models are changed, the homogeneity is not lost where the mass as a function of extensive variables is of order one and the rest zero. We see a similarity in the <span>\\\\(\\\\mu \\\\)</span>–<i>C</i> process across the entropy models signally some universality across entropy models as well as different types of black holes studied before. Finally, we do not see a new universality class for modified entropy as it is seen in studies done for alternate gravity models.\\n</p></div>\",\"PeriodicalId\":578,\"journal\":{\"name\":\"General Relativity and Gravitation\",\"volume\":\"57 5\",\"pages\":\"\"},\"PeriodicalIF\":2.1000,\"publicationDate\":\"2025-05-04\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"General Relativity and Gravitation\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1007/s10714-025-03413-1\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"General Relativity and Gravitation","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s10714-025-03413-1","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

摘要

利用受限相空间(RPST)的形式,对Gibbs-Boltzmann统计和rsamunyi统计的4D动态AdS黑洞热力学进行了比较研究。在RPST的形式中,不考虑压强和体积,而是考虑中心电荷C和化学势\(\mu \)作为热力学变量。磁荷\(\tilde{Q}_m\)的加入使热力学研究的相结构更加丰富,它在T-S过程中增加了一个从不稳定的小黑洞到稳定黑洞的非平衡转变,在F-T和范德华相变和超流体\(\lambda \)相变之上增加了一个霍金-佩奇和戴维斯型相变。我们研究了一个额外的混合系综(\(\tilde{\Phi }_e,\tilde{Q}_m)\)),因为包含\(\tilde{Q}_m\),我们看到Van der Waals相变,其图随着熵模型的变化而变化。对于等压过程,我们看到Bekenstein-Hawking熵中有霍金-佩奇相变,而在r尼熵结构中没有霍金-佩奇相变。我们观察到一个有趣的现象,即改变rsamnyi参数\(\lambda \)时,T-S过程的变化方式与改变中心电荷C时的变化方式相同,强调了在Bekenstein Hawking熵模型中没有看到的一些相似性。我们观察到与史瓦西黑洞和大正则系综有关的两个电荷都关闭时的图具有相似性。我们可以观察到,随着熵模型的改变,在质量作为广泛变量的函数为一阶而其余为零的情况下,均匀性并没有丧失。我们在\(\mu \) -C过程中看到了熵模型之间的相似性,这表明熵模型之间以及之前研究过的不同类型的黑洞之间存在某种通用性。最后,我们没有看到一个新的修正熵的普适性类,因为它是在研究替代重力模型中看到的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Restricted phase space thermodynamics of dyonic AdS black holes: comparative analysis using different entropy models

Using the restricted phase space (RPST) formalism, we perform a comparative study of 4D dyonic AdS black hole thermodynamics in Gibbs–Boltzmann statistics and Rényi statistics. In RPST formalism, instead of pressure and volume, one considers central charge C and chemical potential \(\mu \) as thermodynamic variables. Inclusion of the magnetic charge \(\tilde{Q}_m\) gives rise to a richer phase structure of the study of thermodynamics by adding a non-equilibrium transition from an unstable small black hole to a stable black hole in the TS processes and a Hawking–Page and Davies type phase transition in the FT and specific heat plots on top of the Van der Waals and superfluid \(\lambda \) phase transitions. We study an extra mixed ensemble (\(\tilde{\Phi }_e,\tilde{Q}_m)\) due to the inclusion of \(\tilde{Q}_m\) where we see Van der Waals phase transition and whose plots change as the entropy model changes meaning for isovoltage processes we see Hawking–Page transition in Bekenstein–Hawking entropy and absence of Hawking–Page in Rényi entropy construct. We observe an interesting phenomenon where changing the Rényi parameter \(\lambda \), the TS process changes the same way as when varying the central charge C underlining some similarity that is not seen in the Bekenstein Hawking entropy model. We observe a similarity between the plots when both charges are turned off relating to the Schwarzschild black hole and the grand-canonical ensemble. One can observe that as the entropy models are changed, the homogeneity is not lost where the mass as a function of extensive variables is of order one and the rest zero. We see a similarity in the \(\mu \)C process across the entropy models signally some universality across entropy models as well as different types of black holes studied before. Finally, we do not see a new universality class for modified entropy as it is seen in studies done for alternate gravity models.

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
General Relativity and Gravitation
General Relativity and Gravitation 物理-天文与天体物理
CiteScore
4.60
自引率
3.60%
发文量
136
审稿时长
3 months
期刊介绍: General Relativity and Gravitation is a journal devoted to all aspects of modern gravitational science, and published under the auspices of the International Society on General Relativity and Gravitation. It welcomes in particular original articles on the following topics of current research: Analytical general relativity, including its interface with geometrical analysis Numerical relativity Theoretical and observational cosmology Relativistic astrophysics Gravitational waves: data analysis, astrophysical sources and detector science Extensions of general relativity Supergravity Gravitational aspects of string theory and its extensions Quantum gravity: canonical approaches, in particular loop quantum gravity, and path integral approaches, in particular spin foams, Regge calculus and dynamical triangulations Quantum field theory in curved spacetime Non-commutative geometry and gravitation Experimental gravity, in particular tests of general relativity The journal publishes articles on all theoretical and experimental aspects of modern general relativity and gravitation, as well as book reviews and historical articles of special interest.
×
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