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- W2103248544 abstract "I develop a theory to account for the cosmic ray spectrum. The essential assumption is that, due to fast convective motions, the free mean path perpendicular to the magnetic field is independent of energy and has the scale of the thickness of the shocked layer. I use the basic concept, that the energetic Cosmic Ray particles are accelerated in a Supernova shock that travels down a stellar wind. Discussion gives a knee energy expression, which leads to a suggestion on the physical origin of the mechanical energy of Supernova explosions, the gravitational potential energy mediated by the angular momentum and the magnetic field. The spectrum below the knee is $E^{-8/3}$. At the knee the particles segregate with particle energy according to their charge. The spectrum beyond the knee is very close to $E^{-3}$. The theory has been checked successfully against air shower data in two subsequent papers (Stanev, Biermann, Gaisser, 1992 preprint; Rachen, Stanev, Biermann, 1992 preprint)." @default.
- W2103248544 created "2016-06-24" @default.
- W2103248544 creator A5064895588 @default.
- W2103248544 date "1993-01-15" @default.
- W2103248544 modified "2023-09-27" @default.
- W2103248544 title "Cosmic Rays I.: The cosmic ray spectrum between 10 TeV and 3 EeV" @default.
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- W2103248544 hasPublicationYear "1993" @default.
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