Black Hole Evaporation in the Klein-Sauter-Heisenberg-Euler Formalism - INSPIRE

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Black Hole Evaporation in the Klein-Sauter-Heisenberg-Euler Formalism

T. Damour
(
- Princeton U. and
- Western Australia U.
)
,
R. Ruffini
(
- Princeton U. and
- Western Australia U.
)

1976

3 pages

Published in:

Phys.Rev.D 14 (1976) 332-334

DOI:

10.1103/PhysRevD.14.332

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Abstract: (APS)

A generalization of the classical approach of barrier penetration introduced by Klein, Sauter, Heisenberg, and Euler to curved spaces endowed with future horizons is given. This technique allows one to recover most directly results obtained by Hawking recently. The treatment here presented encompasses, as special cases, the works of Deruelle and Ruffini, of Damour and Ruffini, and of Nakamura and Sato.

FIELD THEORY
Klein-Gordon equation
ASTROPHYSICS
GRAVITATION: VACUUM POLARIZATION
GRAVITATION: ENERGY
PARTICLE: FLUX
FLUX: PARTICLE
ANTIPARTICLE: FLUX
FLUX: ANTIPARTICLE

References(19)

Figures(0)

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