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Topology of nonlinearly charged black hole chemistry via massive gravity

dc.contributor.authorZhang, Meng-Yao
dc.contributor.authorChen, Hao
dc.contributor.authorHassanabadi, Hassan
dc.contributor.authorLong, Zheng-Wen
dc.contributor.authorYang, Hui
dc.date.accessioned2025-12-05T13:02:30Z
dc.date.available2025-12-05T13:02:30Z
dc.date.issued2023
dc.description.abstractThe classification of critical points of charged topological black holes (TBHs) in anti-de Sitter spacetime (AdS) under the Power Maxwell Invariant (PMI)-massive gravity is accomplished within the framework of black hole chemistry (BHC). Considering the grand canonical ensemble (GCE), we show that d = 4 black hole have only one topological class, whereas d >= 5 black holes belong to two different topology classes. Furthermore, the conventional critical point characterized by negative topological charge coincides with the maximum extreme point of temperature; and the novel critical point featuring opposite topological charge corresponds to theminimum extreme point of temperature. With increasing pressure, new phases emerge at the novel critical point while disappear from the conventional one. Moreover, a atypical van der Waals (vdW) behavior is found in d >= 6 dimensions, and the anomaly disappears at the traditional critical point. In the limit of nonlinearity parameter s -> 1, different topology classes are only obtained in the GCE and they may not exist within the canonical ensemble. With the absence of electric potential Phi, the neutral TBHs share the same topological classification results as the charged TBHs in the GCE of Maxwell-massive gravity.eng
dc.formatp. &quot;Article Number: 773&quot;
dc.identifier.doi10.1140/epjc/s10052-023-11933-w
dc.identifier.issn1434-6044
dc.identifier.obd43880260
dc.identifier.urihttp://hdl.handle.net/20.500.12603/1872
dc.identifier.wos001058637000001
dc.language.isoeng
dc.peerreviewedyes
dc.publicationstatuspostprint
dc.publisherSPRINGER
dc.relation.ispartofEuropean Physical Journal C, volume 83, issue: 8eng
dc.relation.publisherversionhttps://link.springer.com/article/10.1140/epjc/s10052-023-11933-w
dc.rights.accessOpen Access
dc.rights.licenseCC BY
dc.source.urlhttps://link.springer.com/article/10.1140/epjc/s10052-023-11933-w
dc.subjectphase-transitionseng
dc.subjectgravitational collapseeng
dc.subjectcosmological constanteng
dc.subjectthermodynamicseng
dc.subjectsingularitieseng
dc.titleTopology of nonlinearly charged black hole chemistry via massive gravityeng
dc.typearticle

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