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arXiv:1304.1945·v3·High Energy Astrophysical Phenomena

Neutron-Proton-Converter Acceleration Mechanism at Subphotospheres of Relativistic Outflows

Kazumi Kashiyama🇺🇸 · Kohta Murase🇺🇸 · Peter Mészáros🇺🇸

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Abstract

We study a type of particle acceleration that operates via neutron-proton conversion in inelastic nuclear collisions. This mechanism can be expected for relativistic shocks at subphotospheres if relativistic outflows contain neutrons. Using a test-particle approximation, we numerically calculate the energy spectrum and the efficiency of accelerated particles, and show that a good energy fraction of the nucleons can be accelerated. This mechanism may especially be relevant if the shock is radiation-mediated, and it would enhance the detectability of GeV-TeV neutrinos.

Comments: 5 pages, 3 figures, published in PRL (submitted on 04/06/2013)

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