Apparent horizons of an N-black-hole system in a space-time with a cosmological constant

Physical Review D Volume 47 Issue 8 Page 3203-3213 published_at 1993-04-15
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Title ( eng )
Apparent horizons of an N-black-hole system in a space-time with a cosmological constant
Creator
Nakao Ken-ichi
Maeda Kei-ichi
Source Title
Physical Review D
Volume 47
Issue 8
Start Page 3203
End Page 3213
Abstract
We present the analytic solution of N Einstein-Rosen bridges ("N black holes") in the space-time with a cosmological constant Λ and analyze it for one- and two-bridge systems. We discuss the three kinds of apparent horizons: i.e., the black-hole, white-hole, and cosmological apparent horizons. In the case of two Einstein-Rosen bridges, when the "total mass" is larger than a critical value, the black-hole apparent horizon surrounding two Einstein-Rosen bridges is not formed even if the distance is very short. Furthermore, in this case, the cosmological apparent horizon enclosing both bridges does not appear. Hence, it seems that when the "total mass" is very large, the Einstein-Rosen bridges cannot collapse into one black hole unless the "gravitational mass" is released in some way.
NDC
Physics [ 420 ]
Language
eng
Resource Type journal article
Publisher
American Physical Society
Date of Issued 1993-04-15
Rights
Copyright (c) 1993 The American Physical Society
Publish Type Version of Record
Access Rights open access
Source Identifier
[ISSN] 1550-7998
[DOI] 10.1103/PhysRevD.47.3203
[NCID] AA00773624
[DOI] http://dx.doi.org/10.1103/PhysRevD.47.3203