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Unstable relics as a source of galactic positrons

Author
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
Source

Physics letters. Section B. 2005, Vol 605, Num 1-2, pp 15-25, 11 p ; ref : 21 ref

CODEN
PYLBAJ
ISSN
0370-2693
Scientific domain
Theoretical physics
Publisher
Elsevier Science, Amsterdam
Publication country
Netherlands
Document type
Article
Language
English
Keyword (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
Keyword (en)
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
Keyword (es)
Bulbo galáctico Materia oscura fría Partícula seudoescalar
Classification
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)

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
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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