Hawking Radiation of Weyl Neutrinos in a Rectilinearly Non-uniformly Accelerating Kinnersley Black Hole

Simple item page
dc.creator-Qing, Wu Shuang
dc.creatorXu, Cai
dc.date2002-04-02
dc.date.accessioned2026-07-07T03:26:46Z
dc.date.available2026-07-07T03:26:46Z
dc.descriptionQuantum thermal effect of Weyl neutrinos in a rectilinearly non-uniformly accelerating Kinnersley black hole is investigated by using the generalized tortoise coordinate transformation. The equation that determines the location, the Hawking temperature of the event horizon and the thermal radiation spectrum of neutrinos are derived. Our results show that the location and the temperature of the event horizon depend not only on the time but also on the angle.
dc.description9 pages, no figure, Latex 2.09, accepted for Chinese Physics Vol. 11, No. 7 (2002)
dc.identifierhttps://arxiv.org/abs/gr-qc/0204005
dc.identifierhttp://arxiv.org/abs/gr-qc/0204005
dc.identifierChin.Phys. 11 (2002) 661-665
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34178
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHawking Radiation of Weyl Neutrinos in a Rectilinearly Non-uniformly Accelerating Kinnersley Black Hole
dc.typetext

Files

Collections

arXiv