QUANTUM-THEORY OF BLACK-HOLES

被引：32

作者：

GEGENBERG, J

KUNSTATTER, G

机构：

[1] UNIV WINNIPEG, INST THEORET PHYS, WINNIPEG R3B 2E9, MANITOBA, CANADA

[2] UNIV WINNIPEG, DEPT PHYS, WINNIPEG R3B 2E9, MANITOBA, CANADA

来源：

PHYSICAL REVIEW D | 1993年 / 47卷 / 10期

关键词：

D O I：

10.1103/PhysRevD.47.R4192

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A solvable two-dimensional conformally invariant midisuperspace model for black holes is obtained by imposing spherical symmetry in four-dimensional conformally invariant Einstein gravity. The Wheeler-DeWitt equation for the theory is solved exactly to obtain the unique quantum wave functional for an isolated black hole with a fixed mass. By suitably relaxing the boundary conditions, a nonperturbative ansatz is obtained for the wave functional of a black hole interacting with its surroundings.

引用

页码：R4192 / R4195

页数：4

共 23 条

[1] 2-DIMENSIONAL QUANTUM-GRAVITY IN MINKOWSKI SPACE [J].