Hawking radiation for twisted complex scalar fields on the Reissner-Nordström black holes and Dirac monopoles

Details Hawking radiation for twisted complex scalar fields on the Reissner-Nordström black holes and Dirac monopoles Hawking radiation for twisted complex scalar fields on the Reissner-Nordström black holes and Dirac monopoles

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997nuphb.486..371g&link_type=abstract

Nuclear Physics B, v. 486, p. 371-389.

Physics

Nuclear Physics

15

Scientific paper

We study, both analytically and numerically, the contribution of the twisted topologically inequivalent configurations (TICs) of complex scalar fields on the Reissner-Nordström black holes to the Hawking radiation. Physically this contribution is conditioned by the natural presence of the Dirac monopoles on the black holes. When neglecting the own (external) electric field of black hole it is established that while increasing the black hole electric charge Q to the extremal value Q = M (M is the black hole mass), the given contribution to the total luminosity (summed up over all the TICs) of the black hole decreases (from the one of order 17% at Q = 0) up to 0. At this value the total luminosity itself tends to 0.

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