Black Holes in brane worlds

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dc.creatorSuranyi, P.
dc.creatorWijewardhana, L. C. R.
dc.date2002-07-09
dc.date.accessioned2026-07-07T04:13:50Z
dc.date.available2026-07-07T04:13:50Z
dc.descriptionIn a Randall-Sundrum theory (RS1) 3+1 dimensional black holes and higher dimensional black holes are not the natural continuations of each other. 3+1 dimensional black holes decay into a large number of 4+1 dimensional black holes at a critical mass, $M_{\rm crit}\sim 10^{32}$ TeV. Those black holes themselves may become unstable above another, albeit much smaller critical mass, $M_0\sim 10^3$TeV.
dc.description8 pages
dc.identifierhttps://arxiv.org/abs/hep-th/0207084
dc.identifierhttp://arxiv.org/abs/hep-th/0207084
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/51405
dc.subjectHigh Energy Physics - Theory
dc.titleBlack Holes in brane worlds
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