| 書目名稱 | Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators |
| 編輯 | Silvia Celli |
| 視頻video | http://file.papertrans.cn/381/380612/380612.mp4 |
| 概述 | Nominated as an outstanding Ph.D. thesis by the Gran Sasso Science Institute, L’Aquila, Italy.Provides a comprehensive review of the search for Galactic cosmic-ray sources.Presents technical descripti |
| 叢書名稱 | Springer Theses |
| 圖書封面 |  |
| 描述 | 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. |
| 出版日期 | Book 2019 |
| 關(guān)鍵詞 | The Origin of Cosmic Rays; Galactic Cosmic-Ray Pevatrons; Supernova Remnants; The Galactic Center regio |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-3-030-33124-5 |
| isbn_softcover | 978-3-030-33126-9 |
| isbn_ebook | 978-3-030-33124-5Series ISSN 2190-5053 Series E-ISSN 2190-5061 |
| issn_series | 2190-5053 |
| copyright | Springer Nature Switzerland AG 2019 |
|Archiver|手機版|小黑屋|
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