Hawking radiation from the Schwarzschild black hole with a global monopole via gravitational anomaly

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dc.creatorPeng, Jun-Jin
dc.creatorWu, Shuang-Qing
dc.date2007-05-09
dc.date2007-07-11
dc.date.accessioned2026-07-07T11:41:06Z
dc.date.available2026-07-07T11:41:06Z
dc.descriptionHawking flux from the Schwarzschild black hole with a global monopole is obtained by using Robinson and Wilczek's method. Adopting a dimension reduction technique, the effective quantum field in the (3+1)--dimensional global monopole background can be described by an infinite collection of the (1+1)--dimensional massless fields if neglecting the ingoing modes near the horizon, where the gravitational anomaly can be cancelled by the (1+1)--dimensional black body radiation at the Hawking temperature.
dc.description4 pages, no figure, 3nd revsion with one reference added
dc.identifierhttps://arxiv.org/abs/0705.1225
dc.identifierhttp://arxiv.org/abs/0705.1225
dc.identifierChin.Phys.B17:825-828,2008
dc.identifierdoi:10.1088/1674-1056/17/3/016
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200417
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHawking radiation from the Schwarzschild black hole with a global monopole via gravitational anomaly
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