Black hole gravitohydromagnetics /

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Bibliographic Details
Author / Creator:Punsly, Brian, 1956-
Imprint:Berlin ; New York : Springer, c2001.
Description:xii, 400 p. : ill. (some col.) ; 24 cm.
Language:English
Series:Astronomy and astrophysics library, 0941-7834
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Format: Print Book
URL for this record:http://pi.lib.uchicago.edu/1001/cat/bib/4451999
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ISBN:3540414665 (alk. paper)
Notes:Includes bibliographical references (p. [387]-391) and index.
Description
Summary:A new branch of physics, black hole gravitohydromagnetics (GHM) is developed from the rudiments to the frontiers of research. GHM describes plasma interactions that combine the effects of gravity and a strong magnetic field, in the vicinity (ergosphere) of a rapidly rotating black hole. This topic was created in response to the astrophysical quest to understand the central engines of radio loud extragalactic radio sources. The theory describes a "torsional tug of war" between rotating ergospheric plasma and the distant asymptotic plasma that extracts the rotational inertia of the black hole.
Physical Description:xii, 400 p. : ill. (some col.) ; 24 cm.
Bibliography:Includes bibliographical references (p. [387]-391) and index.
ISBN:3540414665