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Quantum evolution of near-extremal Reissner-Nordstrom black holes

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Quantum evolution of near-extremal Reissner-Nordstrom black holes

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dc.contributor.author Fabbri, Alessandro
dc.contributor.author Navarro Sanz, Diego José
dc.contributor.author Navarro Salas, José
dc.date.accessioned 2014-03-21T12:13:43Z
dc.date.available 2014-03-21T12:13:43Z
dc.date.issued 2001
dc.identifier.citation Fabbri, A. Navarro Sanz, Diego José Navarro Salas, José 2001 Quantum evolution of near-extremal Reissner-Nordstrom black holes Nuclear Physics B 595 1-2 381 401
dc.identifier.uri http://hdl.handle.net/10550/33650
dc.description.abstract We study the near-horizon AdS_2\timesS^2 geometry of evaporating near-extremal Reissner-Nordstrom black holes interacting with null matter. The non-local (boundary) terms t_{\pm}, coming from the effective theory corrected with the quantum Polyakov-Liouville action, are treated as dynamical variables. We describe analytically the evaporation process which turns out to be compatible with the third law of thermodynamics, i.e., an infinite amount of time is required for the black hole to decay to extremality. Finally we comment briefly on the implications of our results for the information loss problem.
dc.relation.ispartof Nuclear Physics B, 2001, vol. 595, num. 1-2, p. 381-401
dc.subject Partícules (Física nuclear)
dc.subject Camps, Teoria quàntica de
dc.title Quantum evolution of near-extremal Reissner-Nordstrom black holes
dc.type journal article es_ES
dc.date.updated 2014-03-21T12:13:43Z
dc.identifier.doi 10.1016/S0550-3213(00)00661-1
dc.identifier.idgrec 035530
dc.rights.accessRights open access es_ES
dc.identifier.url 10.1016/S0550-3213(00)00661-1

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