Bulk shape of brane-world black holes

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dc.creatorCasadio, Roberto
dc.creatorMazzacurati, Lorenzo
dc.date2002-05-30
dc.date2003-02-18
dc.date.accessioned2026-07-07T11:29:57Z
dc.date.available2026-07-07T11:29:57Z
dc.descriptionWe propose a method to extend into the bulk asymptotically flat static spherically symmetric brane-world metrics. We employ the multipole (1/r) expansion in order to allow exact integration of the relevant equations along the (fifth) extra coordinate and make contact with the parameterized post-Newtonian formalism. We apply our method to three families of solutions previously appeared as candidates of black holes in the brane world and show that the shape of the horizon is very likely a flat ``pancake'' for astrophysical sources.
dc.description10 pages, MPLA style, 5 figures, accepted for publication in MPLA
dc.identifierhttps://arxiv.org/abs/gr-qc/0205129
dc.identifierhttp://arxiv.org/abs/gr-qc/0205129
dc.identifierMod.Phys.Lett.A18:651-660,2003
dc.identifierdoi:10.1142/S0217732303009794
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196880
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleBulk shape of brane-world black holes
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