The conical singularity method and the energy-momentum tensor near the black hole horizon using the Kruskal coordinates

Simple item page
dc.creatorAlves, M.
dc.date2007-04-16
dc.date.accessioned2026-07-07T11:20:17Z
dc.date.available2026-07-07T11:20:17Z
dc.descriptionWe apply the conical singularity method to the two dimensional version of the Schwarzschild metric to obtain the Kruskal coordinates of the black hole in a very simple and direct way. Then we make use of this metric in an approximated version and calculate the expected value of energy-momentum tensor of a massless quantum field near the horizon, resulting in regular expressions for its components.
dc.identifierhttps://arxiv.org/abs/0704.2013
dc.identifierhttp://arxiv.org/abs/0704.2013
dc.identifierMod.Phys.Lett.A22:3057-3063,2007
dc.identifierdoi:10.1142/S0217732307023651
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193912
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleThe conical singularity method and the energy-momentum tensor near the black hole horizon using the Kruskal coordinates
dc.typetext

Files

Collections

arXiv