Inertia of Heat in Advective Accretion Disks around Kerr Black Holes | Zendy

Andrei M. Beloborodov | Zendy; M. A. Abramowicz | Zendy; I. D. Novikov | Zendy

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Inertia of Heat in Advective Accretion Disks around Kerr Black Holes

Author(s) -

Andrei M. Beloborodov,

M. A. Abramowicz,

I. D. Novikov

Publication year - 1997

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.376

H-Index - 489

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/304956

Subject(s) - advection , physics , accretion (finance) , inertia , accretion disc , black hole (networking) , intermediate polar , astrophysics , rotating black hole , mechanics , classical mechanics , thermodynamics , white dwarf , stars , computer network , routing protocol , routing (electronic design automation) , computer science , link state routing protocol

In the innermost region of the advective accretion disk orbiting a black holeof high spin, the inertia of heat stored in the accreting gas is comparable tothat of the gas rest mass itself. Accounting for this effect, we deriveadditional terms in the disk structure equations, and show that the heatinertia plays a significant role in the global energy conservation and dynamicsof accretion in the relativistic advective disks.Comment: 6 pages, Latex, submitted to ApJ

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