Super-spinning compact objects generated by thick accretion disks
If astrophysical black hole candidates are the Kerr black holes predicted by General Relativity, the value of their spin parameter must be subject to the theoretical bound a sub(*) [< or =] 1. In this work, we consider the possibility that these objects are either non-Kerr black holes in an alter...
Saved in:
Published in | Journal of cosmology and astroparticle physics Vol. 2013; no. 3; p. 31 |
---|---|
Main Authors | , |
Format | Journal Article |
Language | English |
Published |
United States
01.03.2013
|
Subjects | |
Online Access | Get full text |
Cover
Loading…
Be the first to leave a comment!