TY - BOOK ID - 61157700 TI - Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators PY - 2019 SN - 3030331245 3030331237 PB - Cham : Springer International Publishing : Imprint: Springer, DB - UniCat KW - Astrophysics. KW - Galactic cosmic rays. KW - Cosmic rays KW - Galaxies KW - Astronomical physics KW - Astronomy KW - Cosmic physics KW - Physics KW - Astrophysics and Astroparticles. UR - https://www.unicat.be/uniCat?func=search&query=sysid:61157700 AB - 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. ER -