CORDIS Project
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This project aims to provide theoretical predictions about gamma-ray emissions from supernova remnants, which are thought to be sources of cosmic rays. It focuses on understanding the clumpy nature of gamma-ray emissions at high energies to support the supernova remnant hypothesis.
Diffusive shock acceleration operating at expanding supernova remnant shells is by far the most popular model for the origin of galactic cosmic rays.
Despite the general consensus received by this model, an unambiguous and conclusive proof of the supernova remnant hypothesis is still missing.
In this context, the recent developments in gamma ray astronomy provide us with precious insights into the problem of the origin of galactic cosmic rays, since production of gamma rays is expected both duri…
CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
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