Amount of antiprotons in cosmic rays due to halo neutralino annihilation
- 31 January 1995
- journal article
- Published by Elsevier in Astroparticle Physics
- Vol. 3 (1) , 77-85
- https://doi.org/10.1016/0927-6505(94)00027-z
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This publication has 34 references indexed in Scilit:
- On the neutralino as dark matter candidate. II. Direct detectionAstroparticle Physics, 1994
- Distribution of dark matter in the galaxy and the lower limits for the masses of supersymmetric particlesPhysics Letters B, 1992
- Searching for TeV dark matter by atmospheric Čerenkov techniquesPhysics Letters B, 1992
- Is it possible to detect the gamma-ray line from neutralino-neutralino annihilation?Physics Letters B, 1992
- Lower bound on the neutralino massPhysics Letters B, 1990
- Cosmic ray constraints on the annihilations of relic particles in the galactic haloPhysics Letters B, 1988
- The Lund Monte Carlo for jet fragmentation and e+ e- physics - jetset version 6.3 - an updateComputer Physics Communications, 1987
- The Lund Monte Carlo for jet fragmentation and e+e- physics - jetset version 6.2Computer Physics Communications, 1986
- The mass distribution within our Galaxy - A three component modelThe Astrophysical Journal, 1981
- Cosmic-Ray Proton and Helium Spectra above 50 GeVPhysical Review Letters, 1972