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astro-ph.HE2023
A Minimal Model for Understanding Secondary Cosmic Rays
Ramanath Cowsik, Dawson Huth
We take a phenomenological approach in a minimal model to understand the spectral intensity of secondary cosmic-ray particles like positrons, antiprotons, Lithium, Beryllium and Bo…
astro-ph.HE2023
Mapping the AMS-02 and CALET Data onto the Source Spectra and Residence Times of Galactic Cosmic Rays
Ramanath Cowsik, Dawson Huth
The recent measurements of the spectral intensities of cosmic-ray nuclei have suggested that the ratio of Boron to Carbon nuclei, , comprises two components, which c…