Galactic positrons and electrons from dark matter and astrophysical sources

Lineros, Roberto

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.

Más información

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