General Solution for Self-Gravitating Spherical Null Dust

dc.creatorMikovic, A.
dc.date1997-05-13
dc.date.accessioned2026-07-07T12:30:38Z
dc.date.available2026-07-07T12:30:38Z
dc.descriptionWe find the general solution of equations of motion for self-gravitating spherical null dust as a perturbative series in powers of the outgoing matter energy-momentum tensor, with the lowest order term being the Vaidya solution for the ingoing matter. This is done by representing the null-dust model as a 2d dilaton gravity theory, and by using a symmetry of a pure 2d dilaton gravity to fix the gauge. Quantization of this solution would provide an effective metric which includes the back-reaction for a more realistic black hole evaporation model than the evaporation models studied previously.
dc.description9 pages, Latex, 1 figure
dc.identifierhttps://arxiv.org/abs/gr-qc/9705030
dc.identifierhttp://arxiv.org/abs/gr-qc/9705030
dc.identifierPhys.Rev.D56:6067-6070,1997
dc.identifierdoi:10.1103/PhysRevD.56.R6067
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/216187
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleGeneral Solution for Self-Gravitating Spherical Null Dust
dc.typetext

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