Speaker
Martin Kološ
(Institute of Physics, Silesian University in Opava)
Description
In this short contribution, I will show our recent results
in cosmic ray particle physics and the involvement of our research
group at the Institute of Physics, Silesian University in Opava, in
the CREDO project. I will discuss charged particle acceleration
models, focusing on particle dynamics in the combined gravitational
and magnetic field around a rotating black hole. Application on PeV
cosmic ray source, Sagittarius A* from our Galaxy center, will be
provided.
