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Dynamics of extremal black holes

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Dynamics of extremal black holes

Record Type:	Language materials, printed : Monograph/item
Title/Author:	Dynamics of extremal black holes/ by Stefanos Aretakis.
Author:	Aretakis, Stefanos.
Published:	Cham :Springer International Publishing : : 2018.,
Description:	xiii, 131 p. :ill. (some col.), digital ; : 24 cm.;
Contained By:	Springer eBooks
Subject:	Black holes (Astronomy) -
Online resource:	https://doi.org/10.1007/978-3-319-95183-6
ISBN:	9783319951836

Dynamics of extremal black holes
Aretakis, Stefanos.

Dynamics of extremal black holes[electronic resource] /by Stefanos Aretakis. - Cham :Springer International Publishing :2018. - xiii, 131 p. :ill. (some col.), digital ;24 cm. - SpringerBriefs in mathematical physics,v.332197-1757 ;. - SpringerBriefs in mathematical physics ;v.2..

This Brief presents in a self-contained, non-technical and illustrative fashion the state-of-the-art results and techniques for the dynamics of extremal black holes. Extremal black holes are, roughly speaking, either maximally rotating or maximally charged. Astronomical observations suggest that near-extremal (stellar or supermassive) black holes are ubiquitous in the universe. The book presents various recently discovered characteristic phenomena (such as the horizon instability) that have enhanced our understanding of the dynamics of extremal black holes. The topics should be of interest to pure mathematicians, theoretical physicists and astronomers. This book provides common ground for communication between these scientific communities.

ISBN: 9783319951836

Standard No.: 10.1007/978-3-319-95183-6doiSubjects--Topical Terms:

672993
Black holes (Astronomy)

LC Class. No.: QB843.B55 / A748 2018

Dewey Class. No.: 523.8875

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300 $a xiii, 131 p. : $b ill. (some col.), digital ; $c 24 cm.
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520 $a This Brief presents in a self-contained, non-technical and illustrative fashion the state-of-the-art results and techniques for the dynamics of extremal black holes. Extremal black holes are, roughly speaking, either maximally rotating or maximally charged. Astronomical observations suggest that near-extremal (stellar or supermassive) black holes are ubiquitous in the universe. The book presents various recently discovered characteristic phenomena (such as the horizon instability) that have enhanced our understanding of the dynamics of extremal black holes. The topics should be of interest to pure mathematicians, theoretical physicists and astronomers. This book provides common ground for communication between these scientific communities.
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