Particle acceleration and radiation processes in supernova remnants.

9 Jun 2021, 12:55
15m
Zoom (Online)

Zoom

Online

Original TeV-PeV gamma rays TeV-PeV gamma rays

Speaker

Vladimir Zirakashvili (Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation, Moscow, Russia)

Description

Diffusive shock acceleration and production of non-thermal emission in galactic supernova remnants is briefly reviewed. We describe gamma ray and X-ray observational features of young and old remnants. The corresponding discussion of Galactic cosmic ray origin is given.

Primary author

Vladimir Zirakashvili (Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation, Moscow, Russia)

Presentation Materials