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- W208300512 abstract "Neutrino astronomy shares with (upgamma )-ray astronomy the objective of understanding the sources and mechanisms of CR acceleration. Due to their much larger interaction cross section, (upgamma )-rays are easier to detect than neutrinos, and (upgamma )-ray astronomy is having a fundamental importance on several topical areas of modern astrophysics and cosmology. The existence of CR sources seems to guarantee the existence of high-energy neutrino sources, in addition to those of (upgamma )-rays. While (upgamma )-rays can be produced both by hadronic (through (pi ^0) decay) or leptonic processes (inverse Compton, bremsstrahlung), neutrinos can only be produced by hadronic processes ((pi ^{pm }) decay), Sect. 10.1." @default.
- W208300512 created "2016-06-24" @default.
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- W208300512 date "2014-10-07" @default.
- W208300512 modified "2023-09-26" @default.
- W208300512 title "High-Energy Neutrino Astrophysics" @default.
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- W208300512 doi "https://doi.org/10.1007/978-3-319-08051-2_10" @default.
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