NON-SMOOTHNESS OF EVENT HORIZONS OF ROBINSON-TRAUTMAN BLACK-HOLES

被引：46

作者：

CHRUSCIEL, PT

SINGLETON, DB

机构：

[1] Australian National University, Canberra, 2601, A.C.T.

[2] Institute of Mathematics, Polish Academy of Sciences, Warsaw, 2601, A.C.T.

来源：

COMMUNICATIONS IN MATHEMATICAL PHYSICS | 1992年 / 147卷 / 01期

关键词：

D O I：

10.1007/BF02099531

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

It is shown that generic "small data" Robinson-Trautman space-times cannot be C123 extended beyond the "r = 2m Schwarzschild-like" event horizon. This implies that an observer living in such a space-time can determine by local measurements whether or not he has crossed the event-horizon of the black-hole.

引用

页码：137 / 162

页数：26

共 25 条

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[2]

BICAK J, 1989, PHYS REV D, V40, P1872

[3]

BOURGUIGNON JP, 1975, COMPOS MATH, V30, P1

[4]

Chavel I., 1984, EIGENVALUES RIEMANNI