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Titlebook: Astroparticle Physics: Theory and Phenomenology; Günter Sigl Book 2017 Atlantis Press and the author(s) 2017 High Energy Astroparticle Phy

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樓主: fitful
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發(fā)表于 2025-3-23 12:28:30 | 只看該作者
12#
發(fā)表于 2025-3-23 15:26:46 | 只看該作者
2.4 CO2 removal and deposition,ncludes the development of the most relevant aspects of air shower physics. The second part then summarizes the current experimental situation and the main open questions, roughly separated for cosmic radiation of Galactic and extragalactic origin. The following chapters will then provide the theore
13#
發(fā)表于 2025-3-23 21:41:24 | 只看該作者
2.3.7 Drilling, completion and production,ies observed in the cosmic radiation arriving at Earth, and possibly beyond. We start with an overview of the main acceleration mechanisms and then discuss the maximal energy that can be reached by these processes. In the last section we then apply this to Galactic and extragalactic source models. T
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發(fā)表于 2025-3-23 23:39:34 | 只看該作者
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發(fā)表于 2025-3-24 04:33:24 | 只看該作者
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發(fā)表于 2025-3-24 09:00:50 | 只看該作者
2.4 CO2 removal and deposition, such as the production of neutral pions and their subsequent decays into .-rays, high energy extraterrestrial neutrinos are unique messengers of hadronic acceleration processes because they can only be produced by the decay of charged pions or heavier mesons which can not be produced electromagneti
17#
發(fā)表于 2025-3-24 12:44:19 | 只看該作者
18#
發(fā)表于 2025-3-24 17:33:49 | 只看該作者
2.4 CO2 removal and deposition,ion of neutrino oscillations in the laboratory. The central third part of this chapter describes how neutrino oscillations are influenced by the presence of matter. This includes both ordinary matter made up of electrons and nuclei, and the role of self-interactions of neutrinos which becomes releva
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發(fā)表于 2025-3-24 19:15:11 | 只看該作者
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發(fā)表于 2025-3-24 23:28:09 | 只看該作者
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