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...

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Bibliographic Details
Published inJournal of cosmology and astroparticle physics Vol. 2013; no. 3; p. 31
Main Authors Li, Zilong, Bambi, Cosimo
Format Journal Article
LanguageEnglish
Published United States 01.03.2013
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