On the stability of two-dimensional extremal black holes

dc.creatorMyung, Y. S.
dc.date1995-10-18
dc.date.accessioned2026-07-07T04:21:33Z
dc.date.available2026-07-07T04:21:33Z
dc.descriptionWe discuss the stability of the extremal ground states of a two-dimensional (2D) charged black hole which carries both electric ($Q_E$) and magnetic ($Q_M$) charges. The method is first to find the physical field and then to derive the equation of the Schrödinger type. It is found that the presenting potential to an on-coming tachyon (as a spectator) takes a barrier-well type. This provides the bound state solution, which implies an exponentially growing mode with respect to time. The 2D extremal ground states all are classically unstable. We conclude that the 2D extremal charged black holes are not considered as the candidates for the stable endpoint of the Hawking evaporation.
dc.description12 pages 2 figures, RevTeX, to obtain figures contact author (ysmyung@physics.inje.ac.kr)
dc.identifierhttps://arxiv.org/abs/hep-th/9510126
dc.identifierhttp://arxiv.org/abs/hep-th/9510126
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/54366
dc.subjectHigh Energy Physics - Theory
dc.titleOn the stability of two-dimensional extremal black holes
dc.typetext

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