Neutron star formation on magnetorotational supernova explosion

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Dr Sergey Moiseenko (Space Research Institute)


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)


Prof. Bisnovtayi-Kogan Gennadi (Space Research Institute)

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