Hot pair-dominated accretion disks

Details Hot pair-dominated accretion disks Hot pair-dominated accretion disks

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...394..500b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 394, no. 2, Aug. 1, 1992, p. 500-514. Research supported by NORDITA, Icelan

Statistics

Computation

35

Accretion Disks, Electron-Positron Pairs, Pair Production, Astronomical Models, Bremsstrahlung, Computational Astrophysics, High Temperature

Scientific paper

The structure and properties of geometrically thin steady hot two-temperature accretion disks, where Comptonized bremsstrahlung is the dominant emission mechanism, are analyzed using a new method based on the fact that the disk solutions depend on two parameters only. The method allows all possible local disk solutions to be displayed as a surface in a single figure. Local disk solutions are found for all accretion rates, viscosity parameters, and radii. As an example, disk solutions are presented for two particular values of the viscosity parameter, 0.1 and 2.0. The existence of global disk solutions is also discussed.

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