Explicit algebraic expressions for cosmic ray electron number density as a function of position and energy are derived for axisymmetric source distributions in galaxies.
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3 Pith papers cite this work. Polarity classification is still indexing.
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A two-component Galactic source model with supernova remnants below 100 TeV and microquasars above, using charge-dependent cutoffs, accounts for cosmic-ray spectra, composition, and the all-particle spectrum up to PeV energies while ruling out nuclei-dependent cutoffs.
citing papers explorer
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The Distribution of Cosmic Ray Electrons in Star-Forming Galaxies
Explicit algebraic expressions for cosmic ray electron number density as a function of position and energy are derived for axisymmetric source distributions in galaxies.
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Two kinds of Galactic source populations could explain the cosmic-ray observation up to the "knee" region
A two-component Galactic source model with supernova remnants below 100 TeV and microquasars above, using charge-dependent cutoffs, accounts for cosmic-ray spectra, composition, and the all-particle spectrum up to PeV energies while ruling out nuclei-dependent cutoffs.
- On The Nonthermal Power Laws In Magnetized Turbulent Plasmas