Titlebook: Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators; Silvia Celli Book 2019 Springer Nature Switzerland AG 2019 The Orig

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https://doi.org/10.1007/978-3-030-33124-5The Origin of Cosmic Rays; Galactic Cosmic-Ray Pevatrons; Supernova Remnants; The Galactic Center regio

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2190-5053 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.978-3-030-33126-9978-3-030-33124-5Series ISSN 2190-5053 Series E-ISSN 2190-5061

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Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators

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Propagation and Radiation of Accelerated Particles in Supernova Remnants with Clumpy Structures,nerally done on a case by case basis. The case of RX J1713.7-3946 is of special interest in this respect. This remnant has been considered for long time the best candidate for an efficient acceleration scenario, mainly due to its high gamma-ray flux. The detection of gamma-ray emission in the energy

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The Galactic Center Region,ee [126] for an extensive review). It is now in a state of relative inactivity [201] but it might well be a non-stationary source. For instance, there are interesting hints of a much stronger emission few hundreds years ago [154]; on the timescale of . years, major variability episodes are expected

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