Singularities in Reissner-Nordstrom black holes

被引：15
|
作者：
Chesler, Paul M. [1 ]
Narayan, Ramesh [1 ,2 ]
Curiel, Erik [1 ,3 ]
机构：
[1] Harvard Univ, Black Hole Initiat, Cambridge, MA 02138 USA
[2] Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[3] Ludwig Maximilians Univ Munchen, Munich Ctr Math Philosophy, Ludwigstr 31, D-80539 Munich, Germany
来源：
CLASSICAL AND QUANTUM GRAVITY | 2020年 / 37卷 / 02期
关键词：
singularities; gravitational collapse; black hole; RELATIVISTIC GRAVITATIONAL COLLAPSE; MASS-INFLATION; CAUCHY-HORIZON; NONSPHERICAL PERTURBATIONS; NULL SINGULARITY; INNER STRUCTURE; SCALAR; INSTABILITY; EVOLUTION; INTERIOR;
D O I：
10.1088/1361-6382/ab5b69
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We study black holes produced via collapse of a spherically symmetric charged scalar field in asymptotically flat space. We employ a late time expansion and argue that decaying fluxes of radiation through the event horizon imply that the black hole must contain a null singularity on the Cauchy horizon and a central spacelike singularity.
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页数：15
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