Speaker
Nikolai Maltsev
Description
The electrons are assumed to be attached to the magnetic field lines of low mass black holes (10^(-3) – 1 Solar Mass). Their acceleration by relativistic centrifugal force is studied. The main factors limiting their maximal energies are considered to be the Inverse Compton effect, Larmor radiation and the inability of low magnetic field to hold high energy electrons. These effects are numerically analysed and based on that the behaviour of an electron with certain initial conditions is studied.
