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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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樓主: 貪吃的人
11#
發(fā)表于 2025-3-23 12:46:29 | 只看該作者
Grundlagen, Kompetenzen und Rollen,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
12#
發(fā)表于 2025-3-23 15:21:03 | 只看該作者
Einleitung. Die Ausnutzung der Atomenergie,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
13#
發(fā)表于 2025-3-23 20:33:55 | 只看該作者
https://doi.org/10.1007/978-3-662-64847-6d by the H.E.S.S. [83], MAGIC [50], VERITAS [139] and HAWC [17] Collaborations. Recently, success has been reported also in neutrino astronomy by the detection of a diffuse flux of multi-TeV neutrinos of ‘extra-terrestrial origin’? by the IceCube Collaboration [2]. In the feasible future, the upgrad
14#
發(fā)表于 2025-3-23 23:34:14 | 只看該作者
Angewandte Regressionsanalyse mit SPSSand VHE gamma-ray and neutrino astronomy. This comes as a result of the fact that the sources of CRs are also expected to be bright VHE gamma-ray and neutrino emitters, due to the decay of neutral and charged pions produced in the interactions between the accelerated particles and the gas surroundin
15#
發(fā)表于 2025-3-24 04:12:32 | 只看該作者
978-3-030-33126-9Springer Nature Switzerland AG 2019
16#
發(fā)表于 2025-3-24 10:20:32 | 只看該作者
17#
發(fā)表于 2025-3-24 13:57:07 | 只看該作者
Angewandte Psychologie im UnternehmenUnderstanding the escape mechanism?of accelerated particles is a key ingredient to establishing a connection between SNRs and the origin of CRs.
18#
發(fā)表于 2025-3-24 16:58:28 | 只看該作者
Particle Escape from Supernova Remnants,Understanding the escape mechanism?of accelerated particles is a key ingredient to establishing a connection between SNRs and the origin of CRs.
19#
發(fā)表于 2025-3-24 20:46:11 | 只看該作者
Silvia CelliNominated 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
20#
發(fā)表于 2025-3-24 23:29:54 | 只看該作者
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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