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dc.contributor.authorWen, Wen-Yuen_US
dc.contributor.authorWu, Shang-Yuen_US
dc.date.accessioned2019-04-03T06:44:52Z-
dc.date.available2019-04-03T06:44:52Z-
dc.date.issued2015-12-21en_US
dc.identifier.issn1434-6044en_US
dc.identifier.urihttp://dx.doi.org/10.1140/epjc/s10052-015-3841-7en_US
dc.identifier.urihttp://hdl.handle.net/11536/129526-
dc.description.abstractThe solution of a remnant was suggested for the black hole ground state after surface gravity is corrected for the loop quantum effect. On the other hand, a Schwarzschild black hole in asymptotic anti-de Sitter space would tunnel into the thermal soliton solution known as the Hawking-Page phase transition. In this letter, we investigate the low temperature phase of a three-dimensional Banados-Teitelboim-Zanelli (BTZ) black hole and four-dimensional AdS Schwarzschild black hole. We find that the thermal soliton is energetically favored rather than the remnant solution at low temperature in three dimensions, while a Planck-size remnant is still possible in four dimensions. Though the BTZ remnant seems energetically disfavored, we argue that it is still possible to find in the overcooled phase if strings were present, and its implication is discussed.en_US
dc.language.isoen_USen_US
dc.titleBlack hole remnant in asymptotic anti-de Sitter spaceen_US
dc.typeArticleen_US
dc.identifier.doi10.1140/epjc/s10052-015-3841-7en_US
dc.identifier.journalEUROPEAN PHYSICAL JOURNAL Cen_US
dc.citation.volume75en_US
dc.citation.issue12en_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:000367403700001en_US
dc.citation.woscount1en_US
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