Asymptotic Spectroscopy of Rotating Black Holes

Simple item page
dc.creatorKeshet, Uri
dc.creatorNeitzke, Andrew
dc.date2007-09-11
dc.date2007-09-30
dc.date.accessioned2026-07-07T11:53:07Z
dc.date.available2026-07-07T11:53:07Z
dc.descriptionWe calculate analytically the transmission and reflection amplitudes for waves incident on a rotating black hole in d=4, analytically continued to asymptotically large, nearly imaginary frequency. These amplitudes determine the asymptotic resonant frequencies of the black hole, including quasinormal modes, total-transmission modes and total-reflection modes. We identify these modes with semiclassical bound states of a one-dimensional Schrodinger equation, localized along contours in the complexified r-plane which connect turning points of corresponding null geodesics. Each family of modes has a characteristic temperature and chemical potential. The relations between them provide hints about the microscopic description of the black hole in this asymptotic regime.
dc.descriptionReferences added
dc.identifierhttps://arxiv.org/abs/0709.1532
dc.identifierhttp://arxiv.org/abs/0709.1532
dc.identifierPhys.Rev.D78:044006,2008
dc.identifierdoi:10.1103/PhysRevD.78.044006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/204423
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAsymptotic Spectroscopy of Rotating Black Holes
dc.typetext

Files

Collections

arXiv