Black Hole Horizon in Superstring Inspired D-Dimensional Dilaton Gravity

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dc.creatorVorontsova, E. G.
dc.creatorSharov, G. S.
dc.date2000-12-30
dc.date.accessioned2026-07-07T04:11:11Z
dc.date.available2026-07-07T04:11:11Z
dc.descriptionIn $D$-dimensional dilaton gravitational model stationary Schwarzschild type solutions (centrally symmetrical solutions in vacuum) are obtained. They contain the two-parameter set of solutions: the first parameter is proportional to a central mass and the second one describes intensity of the dilaton field. If the latter parameter equals zero we have pure Schwarzschild solution with the black hole and constant dilaton field. But when the mentioned parameter is non-zero and the dilaton is non-constant, the black hole horizon vanishes.
dc.description5 pages, LaTeX, 1 gif figure. Talk given at XVth International Workshop QFTHEP'2000 Tver, Russia, 14-20 September 2000
dc.identifierhttps://arxiv.org/abs/hep-th/0101004
dc.identifierhttp://arxiv.org/abs/hep-th/0101004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/50486
dc.subjectHigh Energy Physics - Theory
dc.titleBlack Hole Horizon in Superstring Inspired D-Dimensional Dilaton Gravity
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