A Cannonball Model of Cosmic Rays

Simple item page
dc.creatorDe Rujula, A.
dc.date2004-12-07
dc.date.accessioned2026-07-07T03:54:02Z
dc.date.available2026-07-07T03:54:02Z
dc.descriptionI outline a "Cannon-Ball" model of Cosmic Rays in which their distribution in the Galaxy, their total "luminosity", the broken power-law spectra with their observed slopes, the position of the knee(s) and ankle(s), and the alleged variations of composition with energy are all explained in terms of simple and "standard" physics.
dc.description10 pages, 7 figures. To appear in the proceedings of the XIII International Symposium on Very High Energy Cosmic Ray Interactions, Pylos, Greece, 2004
dc.identifierhttps://arxiv.org/abs/hep-ph/0412094
dc.identifierhttp://arxiv.org/abs/hep-ph/0412094
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44077
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleA Cannonball Model of Cosmic Rays
dc.typetext

Files

Collections

arXiv