Unstable relics as a source of galactic positrons
- Autor
- PICCIOTTO, Charles1 ; POSPELOV, Maxim1 2
[1] Department of Physics and Astronomy, University of Victoria, Victoria, BC, V8P 1A1, Canada
[2] Centre for Theoretical Physics, CPES, University of Sussex, Brighton BN1 9QJ, United Kingdom - Fuente
Physics letters. Section B. 2005, Vol 605, Num 1-2, pp 15-25, 11 p ; ref : 21 ref
- CODEN
- PYLBAJ
- ISSN
- 0370-2693
- Campo Científico
- Theoretical physics
- Editor
- Elsevier Science, Amsterdam
- País de la publicación
- Netherlands
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave (fr)
- Abondance Bulbe galactique Cosmologie Désintégration particule Flux particule Lepton Masse neutrino Matière sombre froide Mélangeage Neutrino Particule neutre Source positon Univers primordial Voie lactée Particule pseudoscalaire
- Palabra clave (in)
- Abundance Galactic bulge Cosmology Particle decay Particle flux Leptons Neutrino mass Cold dark matter Mixing Neutrinos Neutral particles Positron sources Early universe Milky Way Pseudoscalar particle
- Palabra clave (es)
- Bulbo galáctico Materia oscura fría Partícula seudoescalar
- Clasificación
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D35 Characteristics and properties of the milky way / 001E03D35J Galactic center, bar, circumnuclear matter, and bulge (including black hole and distance measurements)
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D70 Unidentified sources and radiation outside the solar system / 001E03D70S Cosmic rays (including sources, origin, acceleration, and interactions)
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 16375920
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1016/j.physletb.2004.11.025 
https://dx.doi.org/10.1016/j.physletb.2004.11.025
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