Gamma-ray emission from young supernova remnants: Hadronic or leptonic?

The debate on the nature of the gamma-ray emission from young supernova remnants is still open. Ascribing such emission to hadronic rather than leptonic processes would provide an evidence for the acceleration of protons and nuclei, and this fact would fit with the very popular (but not proven) para...

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Published in:EPJ Web of conferences 2016-01, Vol.121, p.4001
Main Authors: Gabici, Stefano, Aharonian, Felix
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Language:English
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description The debate on the nature of the gamma-ray emission from young supernova remnants is still open. Ascribing such emission to hadronic rather than leptonic processes would provide an evidence for the acceleration of protons and nuclei, and this fact would fit with the very popular (but not proven) paradigm that supernova remnants are the sources of Galactic cosmic rays. Here, we discuss this issue with a particular focus on the best studied gamma-ray-bright supernova remnant: RX J1713.7-3946.
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title Gamma-ray emission from young supernova remnants: Hadronic or leptonic?
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