A new optically thin accretion disk model with powerful electron-positron outflow

Details A new optically thin accretion disk model with powerful electron-positron outflow A new optically thin accretion disk model with powerful electron-positron outflow

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..586..454y&link_type=abstract

RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP Conference Proceedings, Volume 586, pp. 454-456 (2001).

Astronomy and Astrophysics

Astrophysics

Infall, Accretion, And Accretion Disks, Jets And Bursts, Galactic Winds And Fountains, Active And Peculiar Galaxies And Related Systems, Galactic Nuclei, Circumnuclear Matter, And Bulges

Scientific paper

In the two-temperature optically thin accretion disks, it has been believed that pair processes are not important, in general. However by taking into account the effect of escape of created pairs from accretion disks, pair processes become important, and powerful outflows of escaping pairs are formed. When the mass accretion rate becomes as large as a tenth of the Eddington value, most of the viscously dissipated power is extracted by electron-positron outflow. .

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