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[null,"1.","Record Nr.",null,"UNINA9910373930003321"]
[null,null,"Autore",null,"Celli Silvia"]
[null,null,"Titolo",null,"Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators / / by Silvia Celli"]
[null,null,"Pubbl/distr/stampa",null,"Cham : , : Springer International Publishing : , : Imprint : Springer, , 2019"]
[null,null,"ISBN",null,"3-030-33124-5"]
[null,null,"Edizione",null,"[1st ed. 2019.]"]
[null,null,"Descrizione fisica",null,"1 online resource (264 pages)"]
[null,null,"Collana",null,"Springer Theses, Recognizing Outstanding Ph.D. Research, , 2190-5053"]
[null,null,"Disciplina",null,"523.01"]
[{"$nulls":4},"539.7223"]
[null,null,"Soggetti",null,"Astrophysics"]
[{"$nulls":4},"Astrophysics and Astroparticles"]
[null,null,"Lingua di pubblicazione",null,"Inglese"]
[null,null,"Formato",null,"Materiale a stampa"]
[null,null,null,"Livello bibliografico","Monografia"]
[null,null,"Nota di contenuto",null,"Introduction -- Propagation and Radiation of Accelerated Particles In Super-Nova Remnants With Clumpy Structures -- Particle Escape From Supernova Remnants -- The Galactic Center Region -- Sensitivity studies for Gamma-Ray and Neutrino Telescopes -- Summary and Conclusions -- Appendix."]
[null,null,null,"Sommario/riassunto","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."]