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Faddeev-Popov ghosts and (1+1)-dimensional black-hole evaporation

Journal Article · · Physical Review, D (Particles Fields); (United States)
 [1]
  1. Department of Physics, University of California, Santa Barbara, California 93106 (United States)

Recently Callan, Giddings, Harvey, and the author derived a set of one-loop semiclassical equations describing black-hole formation and/or evaporation in two-dimensional dilaton gravity conformally coupled to {ital N} scalar fields. These equations were subsequently used to show that an incoming matter wave develops a black-hole-type singularity at a critical value {phi}{sub cr} of the dilaton field. In this paper a modification to these equations arising from the Faddeev-Popov determinant is considered and shown to have dramatic effects for {ital N}{lt}24, in which case {phi}{sub cr} becomes complex. The {ital N}{lt}24 equations are solved along the leading edge of an incoming matter shock wave and found to be nonsingular. The shock wave arrives at future null infinity in a zero-energy state, gravitationally cloaked by negative-energy Hawking radiation. Static black-hole solutions supported by a radiation bath are also studied. The interior of the event horizon is found to be nonsingular and asymptotic to de Sitter space for {ital N}{lt}24, at least for sufficiently small mass. It is noted that the one-loop approximation is {ital not} justified by a small parameter for small {ital N}. However an alternate theory (with different matter content) is found for which the same equations arise to leading order in an adjustable small parameter.

DOE Contract Number:
FG03-91ER40618
OSTI ID:
7003530
Journal Information:
Physical Review, D (Particles Fields); (United States), Journal Name: Physical Review, D (Particles Fields); (United States) Vol. 46:10; ISSN PRVDA; ISSN 0556-2821
Country of Publication:
United States
Language:
English

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