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High energy spectrum of hot accretion disks

Conference · · AIP Conf. Proc.; (United States)
OSTI ID:6049626
One possible thermal state for matter accretion onto a black hole is the two temperature (T/sub i/ >> T/sub e/) model of Shapiro, Lightman and Eardley. This state may arise of strong ion heating and strong radiative electron cooling combine, and if the ion-electron coupling is due to Coulomb-type processes. In such a case, extremely high ion temperatures are predicted for optically thin accretion onto a Kerr black hole. The energy particle and photon spectrum such a flow would produce are investigated. Proton-proton reactions lead to primary electron, positron and ..gamma.. ray production; the primary electrons (with E approx. 100 MeV) interact with the accretion flow to produce secondary X and ..gamma.. rays. The flow is modeled with the standard spatially and optically thin Kerr accretion disk with ..cap alpha..-viscosity and sub-Eddington accretion flow. Is is found that ion temperatures 10/sup 12/K
Research Organization:
New Mexico Inst. of Mining and Tech., Socorro
OSTI ID:
6049626
Report Number(s):
CONF-830136-
Conference Information:
Journal Name: AIP Conf. Proc.; (United States) Journal Volume: 101
Country of Publication:
United States
Language:
English