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dc.contributor.authorTsai, Yu-Daien_US
dc.contributor.authorWu, X. N.en_US
dc.contributor.authorYang, Yien_US
dc.date.accessioned2019-04-03T06:36:24Z-
dc.date.available2019-04-03T06:36:24Z-
dc.date.issued2012-02-06en_US
dc.identifier.issn2470-0010en_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevD.85.044005en_US
dc.identifier.urihttp://hdl.handle.net/11536/15215-
dc.description.abstractWe study the critical phenomena of Kerr-AdS black hole. Phase structures are observed at different temperatures, T-L, T-c1 and T-c2 with various features. We discuss the thermal stability considering the isothermal compressibility and how phase transitions related to each other. The asymptotic value of the angular momentum also has an implication on separating stable and unstable part. Near critical temperature T-c1, the order parameter is determined to calculate the critical exponents. All the critical exponents (alpha, beta, gamma, delta) = (0, 1/2, 1, 3) are identical to that of mean field systems. We plot the phase diagram near this critical point, and discuss the scaling symmetry of the free energy.en_US
dc.language.isoen_USen_US
dc.titlePhase structure of the Kerr-AdS black holeen_US
dc.typeArticleen_US
dc.identifier.doi10.1103/PhysRevD.85.044005en_US
dc.identifier.journalPHYSICAL REVIEW Den_US
dc.citation.volume85en_US
dc.citation.issue4en_US
dc.citation.spage0en_US
dc.citation.epage0en_US
dc.contributor.department電子物理學系zh_TW
dc.contributor.departmentDepartment of Electrophysicsen_US
dc.identifier.wosnumberWOS:000299943600003en_US
dc.citation.woscount38en_US
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