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Energy accumulating accretion disk orbiting a Kerr black hole
Author(s) -
Paul H. G.
Publication year - 1988
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.2113090427
Subject(s) - physics , accretion disc , accretion (finance) , thin disk , astrophysics , rotating black hole , black hole (networking) , geodesic , classical mechanics , geometry , stars , computer network , routing protocol , routing (electronic design automation) , computer science , link state routing protocol , mathematics
A geometrically thin, energy accumulating $aL‐disk is suggested which orbits a Kerr black hole. With increasing internal forces, the “standard” disks develop into energy accumulating disks. These accumulating disks are geometrically thin as long as their internal forces remain below a certain bound, allowing nearly geodesic orbits.
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