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Title: Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes. II. Spins and Incoming Objects
Authors:
; ; ; ; ; ; ; ;
Award ID(s):
1815461 1831412
Publication Date:
NSF-PAR ID:
10287783
Journal Name:
The Astrophysical Journal
Volume:
903
Issue:
2
Page Range or eLocation-ID:
133
ISSN:
1538-4357
Sponsoring Org:
National Science Foundation
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  1. A bstract We study a family of four-dimensional, asymptotically flat, charged black holes that develop (charged) scalar hair as one increases their charge at fixed mass. Surprisingly, the maximum charge for given mass is a nonsingular hairy black hole with nonzero Hawking temperature. The implications for Hawking evaporation are discussed.