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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Quantum evolution of near-extremal Reissner-Nordstrom black holes

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Fabbri, Alessandro; Navarro Sanz, Diego José; Navarro Salas, José Perfil
Aquest document és un/a article, creat/da en: 2001

Este documento está disponible también en : http://dx.doi.org/10.1016/S0550-3213(00)00661-1
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.

    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
http://dx.doi.org/10.1016/S0550-3213(00)00661-1
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