Asymmetry of Hawking Radiation of Dirac Particles in a Charged Vaidya - de Sitter Black Hole

Simple item page
dc.creatorWu, S. Q.
dc.creatorCai, X.
dc.date2001-04-18
dc.date.accessioned2026-07-07T03:25:50Z
dc.date.available2026-07-07T03:25:50Z
dc.descriptionThe Hawking radiation of Dirac particles in a charged Vaidya - de Sitter black hole is investigated by using the method of generalized tortoise coordinate transformation. It is shown that the Hawking radiation of Dirac particles does not exist for $P_1, Q_2$ components, but for $P_2, Q_1$ components it does. Both the location and the temperature of the event horizon change with time. The thermal radiation spectrum of Dirac particles is the same as that of Klein-Gordon particles.
dc.description10 pages in 12pt Revtex, no figure, to appear in Int. J. Theor. Phys. Vol. 40, No.7 (2001)
dc.identifierhttps://arxiv.org/abs/gr-qc/0104056
dc.identifierhttp://arxiv.org/abs/gr-qc/0104056
dc.identifierInt.J.Theor.Phys. 40 (2001) 1349-1357
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33866
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAsymmetry of Hawking Radiation of Dirac Particles in a Charged Vaidya - de Sitter Black Hole
dc.typetext

Files

Collections

arXiv