Black hole constraints on the running-mass inflation model

2000 ◽  
Vol 62 (4) ◽  
Author(s):  
Samuel M. Leach ◽  
Ian J. Grivell ◽  
Andrew R. Liddle
2011 ◽  
Vol 84 (10) ◽  
Author(s):  
Eric G. Brown ◽  
Robert Mann ◽  
Leonardo Modesto
Keyword(s):  

2011 ◽  
Vol 84 (2) ◽  
Author(s):  
P. P. Avelino ◽  
A. J. S. Hamilton ◽  
C. A. R. Herdeiro ◽  
M. Zilhão

The internal structure of a charged spherical black hole is still a topic of debate. In a non-rotating but aspherical gravitational collapse to form a spherical charged black hole, the backscattered gravitational wave tails enter the black hole and are blueshifted at the Cauchy horizon. This has a catastrophic effect if combined with an outflux crossing the Cauchy horizon: a singularity develops at the Cauchy horizon and the effective mass inflates. Recently, a numerical study of a massless scalar field in the Reissner-Nordström background suggested that a spacelike singularity may form before the Cauchy horizon forms. We will show that there exists an approximate analytic solution of the scalar-field equations which allows the mass-inflation singularity at the Cauchy horizon to exist. In particular, we see no evidence that the Cauchy horizon is preceded by a spacelike singularity.


2003 ◽  
Vol 67 (4) ◽  
Author(s):  
Laura Covi ◽  
David H. Lyth ◽  
Alessandro Melchiorri

1996 ◽  
Vol 53 (12) ◽  
pp. 7373-7376 ◽  
Author(s):  
Alfio Bonanno

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