Evaporation of Near-Extremal Reissner-Nordström Black Holes

Alessandro Fabbri; Diego J. Navarro; José Navarro-Salas

doi:10.1103/PhysRevLett.85.2434

Evaporation of Near-Extremal Reissner-Nordström Black Holes

Alessandro Fabbri, Diego J. Navarro, and José Navarro-Salas

Phys. Rev. Lett. 85, 2434 – Published 18 September 2000

Abstract

The formation of near-extremal Reissner-Nordström black holes in the $S$ -wave approximation can be described, near the event horizon, by an effective solvable model. The corresponding one-loop quantum theory remains solvable and allows one to follow analytically the evaporation process, which is shown to require an infinite amount of time.

Received 10 April 2000

DOI:https://doi.org/10.1103/PhysRevLett.85.2434

Authors & Affiliations

Alessandro Fabbri^*

Dipartimento di Fisica dell'Università di Bologna and INFN sezione di Bologna, Via Irnerio 46, 40126 Bologna, Italy

Diego J. Navarro^† and José Navarro-Salas^‡

Departamento de Física Teórica and IFIC, Centro Mixto Universidad de Valencia-CSIC, Facultad de Física, Universidad de Valencia, Burjassot-46100, Valencia, Spain

^*Email address: fabbria@bo.infn.it
^†Email address: dnavarro@ific.uv.es
^‡Email address: jnavarro@lie.uv.es