Monte Carlo Simulations of Radiation from Compact Objects
Edison Liang, Markus Boettcher, Dechun Lin
We have performed Monte Carlo simulations of x-and-gamma-ray emissions
from accreting weakly magnetized neutron stars and inner disks of
accreting black holes. We will present simulation results for the
emissons from the Alfven radius of a neutron star and hot ion tori
around the black hole horizon, using both internal synchrotron soft
photons and external blackbody photons, and including the effects
of wave turbulence acceleration and Coulomb coupling to virial ions.
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On 16 Jul 1999, 09:19.