Hidden Bibliographic Details
| ISBN: | 9783030331245
3030331245
3030331237
9783030331238
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| Notes: | "Doctoral thesis accepted by the Gran Sasso Science Institute, L'Aquila, Italy."--T.p.
Includes bibliographical references and index.
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| Summary: | This book addresses three "hot" topics concerning the general problem of the origin of Galactic cosmic rays, namely (1) the acceleration, propagation, and radiation of particles in supernova remnants; (2) very high energy neutrinos from the Galactic Center; and (3) the potential held by the next-generation gamma-ray and neutrino detectors CTA and KM3NeT for studying extended non-thermal sources in the Galaxy. The topics are intrinsically connected to determining the nature ("hadronic or leptonic?") of gamma-ray emissions from young and middle-aged supernova remnants and the search for cosmic-ray PeVatrons. The results and conclusions provided here are based on extensive analytical and numerical simulations, which are formulated and presented in a straightforward format that can be readily used in the interpretations of gamma-ray and neutrino observations, as well as for confident predictions for future measurements.
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| Other form: | Original 3030331237 9783030331238
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| Standard no.: | 10.1007/978-3-030-33
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