Speaker
Dr
Vladimir Zirakashvili
(IZMIRAN)
Description
Nonlinear model of diffusive shock acceleration is used for
investigation of the particle acceleration in old supernova remnants
W28 and W44.
We modeled the hydrodynamical evolution of the remnats, shock modification and
streaming instability produced by accelerated particles. Comparison with
avalable radio and gamma-ray data is given.
Primary authors
Dr
Vladimir Ptuskin
(IZMIRAN)
Dr
Vladimir Zirakashvili
(IZMIRAN)
