Dynamics of Extremal Black Holes (eBook)

Artikelnummer: 978-3-319-95183-6
Einband: PDF
Verfügbarkeit: Download, sofort verfügbar (Link per E-Mail)
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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.

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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VerlagSpringer International Publishing
EinbandPDF
Erscheinungsjahr2018
Seitenangabe131 S.
AusgabekennzeichenEnglisch
AbbildungenXIII, 131 p. 82 illus., 62 illus. in color.
Masse5'979 KB
PlattformPDF
ReiheSpringerBriefs in Mathematical Physics; Physics and Astronomy; Physics and Astronomy
AutorAretakis, Stefanos

Alle Bände der Reihe "SpringerBriefs in Mathematical Physics; Physics and Astronomy; Physics and Astronomy (R0)"

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