Approximate Stress Energy Tensor for Evaporating Black Holes - INSPIRE

DataBETA

Approximate Stress Energy Tensor for Evaporating Black Holes

Cenalo Vaz
(
- Johns Hopkins U.
)

Jul, 1988

11 pages

Published in:

Phys.Rev.D 39 (1989) 1776

DOI:

10.1103/PhysRevD.39.1776

Report number:

JHU-TIPAC-8806

View in:

reference search17 citations

Citations per year

Abstract: (APS)

We approximate the Israel-Hartle-Hawking and Unruh stress-energy tensors of quantum fields in the neighborhood of a static Schwarzschild black hole. The approximate tensors are constructed from the conservation equations in the ultrastatic optical metric of the black hole and the expected regularity properties at the horizon, in the respective vacua. Our scheme reproduces the approximation of Page, Brown, and Ottewill for the Israel-Hartle-Hawking vacuum and yields a tensor for the Unruh state. The latter exhibits the correct behavior at infinity and predicts luminosities in good agreement with numerical calculations.

black hole
TENSOR: ENERGY-MOMENTUM
ANOMALY: CONFORMAL
RADIATION: HAWKING

References(13)

Figures(0)

Vacuum Polarization in Schwarzschild Space-Time

P. Candelas
(
- Texas U.
)

- Phys.Rev.D 21 (1980) 2185-2202
•
DOI:
- 10.1103/PhysRevD.21.2185

QUANTUM STRESS TENSOR IN SCHWARZSCHILD SPACE-TIME

K.W. Howard
(
- Texas U.
)
,
P. Candelas
(
- Texas U.
)

- Phys.Rev.Lett. 53 (1984) 403-406
•
DOI:
- 10.1103/PhysRevLett.53.403

VACUUM < T (MU) (NU) > IN SCHWARZSCHILD SPACE-TIME

K.W. Howard
(
- Texas U.
)

- Phys.Rev.D 30 (1984) 2532-2547,
- Phys. Rev. D30 ( 1984) 2532-2547
•
DOI:
- 10.1103/PhysRevD.30.2532

Thermal Stress Tensors in Static Einstein Spaces

Don N. Page
(
- Penn State U.
)

- Phys.Rev.D 25 (1982) 1499
•
DOI:
- 10.1103/PhysRevD.25.1499

EFFECTIVE ACTIONS AND CONFORMAL TRANSFORMATIONS

M.R. Brown
(
- Oxford U.
)
,
A.C. Ottewill
(
- Oxford U.
)

- Phys.Rev.D 31 (1985) 2514-2520,
- Phys. Rev. D31 ( 1985) 2514-2520
•
DOI:
- 10.1103/PhysRevD.31.2514

Killing Approximation for Vacuum and Thermal Stress - Energy Tensor in Static Space-times

Valeri P. Frolov
(
- British Columbia U. and
- Lebedev Inst.
)
,
A.I. Zelnikov
(
- British Columbia U. and
- Lebedev Inst.
)

- Phys.Rev.D 35 (1987) 3031-3044,
- Phys. Rev. D35 ( 1987) 3031-3044
•
DOI:
- 10.1103/PhysRevD.35.3031

Path Integral Derivation of Black Hole Radiance

J.B. Hartle
(
- UC, Santa Barbara and
- Caltech and
- Cambridge U.
)
,
S.W. Hawking
(
- UC, Santa Barbara and
- Caltech and
- Cambridge U.
)

- Phys.Rev.D 13 (1976) 2188-2203
•
DOI:
- 10.1103/PhysRevD.13.2188

Notes on black hole evaporation

W.G. Unruh
(
- McMaster U.
)

- Phys.Rev.D 14 (1976) 870
•
DOI:
- 10.1103/PhysRevD.14.870

Conformally Invariant Quantum Field Theory in Static Einstein Space-times

- Phys.Rev.D 33 (1986) 2840-2850,
- Phys. Rev. D33 ( 1986) 2840-2850
•
DOI:
- 10.1103/PhysRevD.33.2840

Trace Anomalies and the Hawking Effect

S.M. Christensen
(
- King's Coll. London and
- Utah U. and
- Texas A-M
)
,
S.A. Fulling
(
- King's Coll. London and
- Utah U. and
- Texas A-M
)

- Phys.Rev.D 15 (1977) 2088-2104
•
DOI:
- 10.1103/PhysRevD.15.2088

Quantum Field Theory in Curved Space-Time

Bryce S. DeWitt
(
- Texas U.
)

- Phys.Rept. 19 (1975) 295-357
•
DOI:
- 10.1016/0370-1573(75)90051-4

Particle Emission Rates from a Black Hole: Massless Particles from an Uncharged, Nonrotating Hole

Don N. Page
(
- Caltech
)

- Phys.Rev.D 13 (1976) 198-206
•
DOI:
- 10.1103/PhysRevD.13.198

Black Holes Do Evaporate Thermally

James M. Bardeen
(
- Washington U., Seattle
)

- Phys.Rev.Lett. 46 (1981) 382-385
•
DOI:
- 10.1103/PhysRevLett.46.382