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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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发表于 2025-3-21 20:07:27 | 显示全部楼层 |阅读模式
书目名称Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators
编辑Silvia Celli
视频video
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
丛书名称Springer Theses
图书封面Titlebook: Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators;  Silvia Celli Book 2019 Springer Nature Switzerland AG 2019 The Orig
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
关键词The Origin of Cosmic Rays; Galactic Cosmic-Ray Pevatrons; Supernova Remnants; The Galactic Center regio
版次1
doihttps://doi.org/10.1007/978-3-030-33124-5
isbn_softcover978-3-030-33126-9
isbn_ebook978-3-030-33124-5Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer Nature Switzerland AG 2019
The information of publication is updating

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Grundlagen, Kompetenzen und Rollen,unequivocally explain the observations [119, 182, 255]. To address this issue, it has been proposed by Zirakashvili and Aharonian [255] (and later on investigated by [118, 143]) that the very hard energy spectrum at low energies could result also from hadronic emission if the SNR is expanding inside a clumpy medium.
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Book 2019 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 connecte
发表于 2025-3-23 02:32:41 | 显示全部楼层
2190-5053 for Galactic cosmic-ray sources.Presents technical descriptiThis 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
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Personalpsychologie im Projektmanagement in order to provide the reader with a complete picture concerning the current understanding of the physical processes responsible for the formation of the cosmic-ray (CR) flux observed at Earth and the detection principles of their secondary emission.
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