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Evaporation of near-extremal Reissner-Nordstrom black holes

Repositori DSpace/Manakin

dc.contributor.author	Fabbri, Alessandro
dc.contributor.author	Navarro Sanz, Diego José
dc.contributor.author	Navarro Salas, José
dc.date.accessioned	2014-03-27T12:42:20Z
dc.date.available	2014-03-27T12:42:20Z
dc.date.issued	2000
dc.identifier.citation	Fabbri, Alessandro Navarro, Diego J. Navarro Salas, José 2000 Evaporation of near-extremal Reissner-Nordstrom black holes Physical Review Letters 85 12 2434 2437
dc.identifier.uri	http://hdl.handle.net/10550/33725
dc.description.abstract	The formation of near-extremal Reissner-Nordstrom 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 to follow analytically the evaporation process which is shown to require an infinite amount of time.
dc.relation.ispartof	Physical Review Letters, 2000, vol. 85, num. 12, p. 2434-2437
dc.subject	Astrofísica
dc.subject	Camps, Teoria quàntica de
dc.subject	Astronomia
dc.title	Evaporation of near-extremal Reissner-Nordstrom black holes
dc.type	journal article	es_ES
dc.date.updated	2014-03-27T12:42:20Z
dc.identifier.doi	10.1103/PhysRevLett.85.2434
dc.identifier.idgrec	081962
dc.rights.accessRights	open access	es_ES
dc.identifier.url	10.1103/PhysRevLett.85.2434