Evaporation and fate of dilatonic black holes

Jun Ichirou Koga*, Kei Ichi Maeda

*この研究の対応する著者

研究成果: Article査読

44 被引用数 (Scopus)

抄録

We study both spherically symmetric and rotating black holes with dilaton coupling and discuss the evaporation of these black holes via Hawkings quantum radiation and their fates. We find that the dilaton coupling constant drastically affects the emission rates, and therefore the fates of the black holes. When the charge is conserved, the emission rate from the nonrotating hole is drastically changed beyond =1 (a superstring theory) and diverges in the extreme limit. In the rotating cases we analyze the slowly rotating black hole solution with arbitrary as well as three exact solutions: the Kerr-Newman (=0), Kaluza-Klein (= 3), and Sen black hole (=1 and with axion field). Beyond the same critical value of 1, the emission rate becomes very large near the maximally charged limit, while for <1 it remains finite. The black hole with >1 may evolve into a naked singularity due to its large emission rate. We also consider the effects of a discharge process by investigating superradiance for the nonrotating dilatonic black hole.

本文言語English
ページ(範囲)7066-7079
ページ数14
ジャーナルPhysical Review D
52
12
DOI
出版ステータスPublished - 1995
外部発表はい

ASJC Scopus subject areas

  • 物理学および天文学(その他)

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