{"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, 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, 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. 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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。
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 T–S processes and a Hawking–Page and Davies type phase transition in the F–T 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 T–S 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.
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.