Galactic neutrino background from cosmic ray interaction with the ISM content

Details Galactic neutrino background from cosmic ray interaction with the ISM content Galactic neutrino background from cosmic ray interaction with the ISM content

2007-09-03

arxiv.org/abs/0709.0278v2

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figures Proceeding of the 30th International Cosmic Ray Conference, Merida (2007), Yucatan, Mexico

Scientific paper

We use a diffusive model for the propagation of Galactic cosmic rays to
estimate the charged pion production in interactions with protons of the
interstellar medium. Cosmic ray nuclei from proton to iron are considered and
the corresponding contribution to the neutrino secondary flux produced as a
result of spallation is also estimated.

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