Type IIn supernovae as sources of high energy neutrinos
arXiv:1505.08144
Abstract
It is shown that high-energy astrophysical neutrinos observed in the IceCube experiment can be produced by protons accelerated in extragalactic Type IIn supernova remnants by shocks propagating in the dense circumstellar medium. The nonlinear diffusive shock acceleration model is used for description of particle acceleration.
9 pages, 4 figures, oral talk at 34th ICRC, Hague, Netherlands 30July-06Aug 2015