## Abstract We consider a spherically symmetric, double characteristic initial value problem for the (real) EinsteinβMaxwellβscalar field equations. On the initial outgoing characteristic, the data is assumed to satisfy the Price law decay widely believed to hold on an event horizon arising from th
β¦ LIBER β¦
Complete Semiclassical Treatment of the Quantum Black Hole Problem
β Scribed by B. Harms; Y. Leblanc
- Publisher
- Elsevier Science
- Year
- 1995
- Tongue
- English
- Weight
- 399 KB
- Volume
- 244
- Category
- Article
- ISSN
- 0003-4916
No coin nor oath required. For personal study only.
β¦ Synopsis
Two types of semiclassical calculations have been used to study quantum effects in black hole backgrounds, the WKB and the mean field approaches. In this work we systematically reconstruct the logical implications of both methods on quantum black hole physics and provide the link between these two approaches. Our conclusions completely support our previous findings based solely on the WKB method: quantum black holes are effectively (p)-brane excitations and, consequently, no information loss paradox exists in this problem. r: 1995 Acadenic Press. Inc
π SIMILAR VOLUMES
The interior of charged black holes and
β
Mihalis Dafermos
π
Article
π
2005
π
John Wiley and Sons
π
English
β 421 KB
Collisional line broadening in the atmos
β
J. Buldyreva; S. V. Ivanov; L. Nguyen
π
Article
π
2005
π
John Wiley and Sons
π
English
β 118 KB
Complete solution of the free-space spon
β
J. Seke
π
Article
π
1993
π
Elsevier Science
π
English
β 504 KB
Construction of a complete orthogonal sy
π
Article
π
1965
π
Elsevier Science
π
English
β 88 KB