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Type IIn supernovae as sources of high energy neutrinos

Authors :
Zirakashvili, V. N.
Ptuskin, V. S.
Publication Year :
2015
Publisher :
arXiv, 2015.

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.<br />Comment: 9 pages, 4 figures, oral talk at 34th ICRC, Hague, Netherlands 30July-06Aug 2015

Subjects

Subjects :
High Energy Astrophysical Phenomena (astro-ph.HE)
Astrophysics::High Energy Astrophysical Phenomena
Astrophysics::Instrumentation and Methods for Astrophysics
Physics::Accelerator Physics
FOS: Physical sciences
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics - High Energy Astrophysical Phenomena
Astrophysics::Galaxy Astrophysics

Details

Database :
OpenAIRE
Accession number :
edsair.doi.dedup.....23360a0bbe01f4aabc5c05cd6c48340e
Full Text :
https://doi.org/10.48550/arxiv.1505.08144
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