Quantum Thermal Effect of Dirac Particles in a Non-uniformly Rectilinearly Accelerating Black Hole with Electronic Charge, Magnetic Charge and Cosmological Constant

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dc.creatorWu, S. Q.
dc.creatorCai, X.
dc.date2001-12-09
dc.date.accessioned2026-07-07T03:26:30Z
dc.date.available2026-07-07T03:26:30Z
dc.descriptionThe Hawking radiation of Dirac particles in an arbitrarily rectilinearly accelerating Kinnersley black hole with electro-magnetic charge and cosmological constant is investigated by using method of the generalized tortoise coordinate transformation. Both the location and the temperature of the event horizon depend on the time and the polar angle. The Hawking thermal radiation spectrum of Dirac particles is also derived. PACS numbers: 04.70.Dy, 97.60.Lf
dc.description12pt revtex, 11 pages, no figure, to appear in Int. J. Theor. Phys. 41 (2002) No. 4
dc.identifierhttps://arxiv.org/abs/gr-qc/0112014
dc.identifierhttp://arxiv.org/abs/gr-qc/0112014
dc.identifierInt.J.Theor.Phys. 41 (2001) 641-651
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34068
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQuantum Thermal Effect of Dirac Particles in a Non-uniformly Rectilinearly Accelerating Black Hole with Electronic Charge, Magnetic Charge and Cosmological Constant
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