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arXiv · astro-ph/9703045

Gamma-Rays and Neutrinos from Very Young Supernova Remnants

R. J. Protheroe·W. Bednarek·Q. Luo
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Abstract

We consider the result of acceleration of heavy ions in the slot gap potential of a very young pulsar with a hot polar cap. Photodisintegration of the heavy ions in the radiation field of the polar cap and pulsar surface gives rise to a flux of energetic neutrons. Some fraction of these neutrons interact with target nuclei in the supernova shell to produce neutrino and gamma-ray signals which should be observable from very young supernova remnants in our galaxy for a range of pulsar parameters.

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R. J. Protheroe, W. Bednarek, Q. Luo. 1997-09-04. Gamma-Rays and Neutrinos from Very Young Supernova Remnants. https://doi.org/10.1016/s0927-6505(98)00014-0

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