Galactic positrons and electrons from dark matter and astrophysical sources
Abstract
The electron and positron cosmic rays observations have impulsed a hot debate regarding the origin of such particles. Their propagation in the galactic medium is modeled according to a successfully tested two-zone propagation model. The theoretical uncertainties related to their propagation and production are studied for three cases: secondary production, Dark Matter annihilation, and originating from supemovae remnants. (C) 2010 Elsevier B.V. All rights reserved.
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Título según WOS: | ID WOS:000287780800016 Not found in local WOS DB |
Título de la Revista: | NUCLEAR INSTRUMENTS METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT |
Volumen: | 630 |
Número: | 1 |
Editorial: | Elsevier |
Fecha de publicación: | 2011 |
Página de inicio: | 70 |
Página final: | 73 |
DOI: |
10.1016/j.nima.2010.06.030 |
Notas: | ISI |