Speaker
Dr
Sergey Moiseenko
(Space Research Institute)
Description
We present results of formation of protoneutron star as a result of magnetorotational supernova explosion. At the formation stage the magnetic field on the surface of the NS is chaotic and strong ~ 10(14)G. We found oscillations of the NS in simualtions. Details of magnetorotational supernova exlosion mechanism are discussed.
Primary author
Dr
Sergey Moiseenko
(Space Research Institute)
Co-author
Prof.
Bisnovtayi-Kogan Gennadi
(Space Research Institute)
