The lifetime problem of evaporating black holes: mutiny or resignation Carlos Barcel´o1, Ra´ulCarballo-Rubio1, Luis J. Garay2;3, and Gil Jannes4 1 Instituto de Astrof´ısicade Andaluc´ıa(IAA-CSIC), Glorieta de la Astronom´ıa, 18008 Granada, Spain 2 Departamento de F´ısicaTe´oricaII, Universidad Complutense de Madrid, 28040 Madrid, Spain 3 Instituto de Estructura de la Materia (IEM-CSIC), Serrano 121, 28006 Madrid, Spain 4 Modelling & Numerical Simulation Group, Universidad Carlos III de Madrid, Avda. de la Universidad 30, 28911 Legan´es,Spain E-mail:
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[email protected] Abstract. It is logically possible that regularly evaporating black holes exist in nature. In fact, the prevalent theoretical view is that these are indeed the real objects behind the curtain in astrophysical scenarios. There are several proposals for regularizing the classical singularity of black holes so that their formation and evaporation do not lead to information-loss problems. One characteristic is shared by most of these proposals: these regularly evaporating black holes present long-lived trapping horizons, with absolutely enormous evaporation lifetimes in whatever measure. Guided by the discomfort with these enormous and thus inaccessible lifetimes, we elaborate here on an alternative regularization of the classical singularity, previously proposed by the authors in an emergent gravity framework, which leads to a completely different scenario. In our scheme the collapse of a stellar object would result in a genuine time-symmetric bounce, which in geometrical terms amounts to the connection of a black-hole geometry with a white-hole geometry in a regular manner.