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We study neutrino spin oscillations while the particles scatter off arotating black hole surrounded by a thick magnetized accretion disk. Neutrinospin precession is caused by the interaction of the neutrino magnetic momentwith the magnetic field in the disk which has both toroidal and poloidalcomponents. Our calculation of the observed neutrino fluxes, accounting forspin oscillations, are based on numerical simulations of the propagation of agreat number of incoming test particles using High Performance ParallelComputing. The obtained results significantly improve our previous findings. Webriefly discuss the applications for the observations of astrophysicalneutrinos.

Spin oscillations in neutrino gravitational scattering