The virtual black hole in 2d quantum gravity

被引:31
|
作者
Grumiller, D
Kummer, W
Vassilevich, DV
机构
[1] Vienna Tech Univ, Inst Theoret Phys, A-1040 Vienna, Austria
[2] Univ Leipzig, Inst Theoret Phys, D-04109 Leipzig, Germany
基金
俄罗斯基础研究基金会; 奥地利科学基金会;
关键词
D O I
10.1016/S0550-3213(00)00231-5
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
As shown recently (W. Kummer, H. Liebl, D,V. Vassilevich, Nucl, Phys, B 544 (1999) 403) 2d quantum gravity theories - including spherically reduced Einstein-gravity - after an exact path integral of its geometric part can be treated perturbatively in the loops of (scalar) matter. Obviously the classical mechanism of black hole formation should be contained in the tree approximation of the theory. This is shown to be the case for the scattering of two scalars through an intermediate state which by its effective black hole mass is identified as a "virtual black hole". The present discussion is restricted to minimally coupled scalers without and with mass. in the first case the probability amplitude diverges, except the black hole is "plugged" by a suitable boundary condition. For massive scalars a finite S-matrix element is obtained. (C) 2000 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:438 / 456
页数:19
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