Cosmic-ray positron from superparticle dark matter and the PAMELA anomaly
- 25 May 2009
- journal article
- research article
- Published by Elsevier in Physics Letters B
- Vol. 675 (5) , 446-449
- https://doi.org/10.1016/j.physletb.2009.04.049
Abstract
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Funding Information
- Ministry of Education, Culture, Sports, Science and Technology (19540255)
- Japan Society for the Promotion of Science
This publication has 18 references indexed in Scilit:
- Pulsars as the sources of high energy cosmic ray positronsJournal of Cosmology and Astroparticle Physics, 2009
- High energy cosmic rays from the decay of gravitino dark matterPhysical Review D, 2008
- Positrons from dark matter annihilation in the galactic halo: Theoretical uncertaintiesPhysical Review D, 2008
- Non-perturbative effect on thermal relic abundance of dark matterPhysics Letters B, 2007
- PYTHIA 6.4 physics and manualJournal of High Energy Physics, 2006
- Wino cold dark matter from anomaly mediated SUSY breakingNuclear Physics B, 2000
- Out of this world supersymmetry breakingNuclear Physics B, 1999
- Positron propagation and fluxes from neutralino annihilation in the haloPhysical Review D, 1998
- Production and Propagation of Cosmic‐Ray Positrons and ElectronsThe Astrophysical Journal, 1998
- Measurements of the Cosmic-Ray Positron Fraction from 1 to 50 G[CLC]e[/CLC]VThe Astrophysical Journal, 1997