Published August 6, 1984
| Version v1
Journal article
Cosmic-ray antiprotons as a probe of a photino-dominated universe
Creators
- 1. Astronomy Department, University of California, Berkeley, California 94720 and Institute for Theoretical Physics, University of California, Santa Barbara, California 93106
Description
Observational tests of the hypothesis that the universe is flat and dominated by dark matter in the form of massive photinos include the production of significant fluxes of cosmic rays and gamma rays in our galactic halo. Specification of the cosmological photino density and the masses of scalar quarks and leptons determines the present annihilation rate. The predicted number of low-energy cosmic-ray antiprotons is comparable to the observed flux
Additional details
Publishing Information
- Journal Title
- Phys. Rev. Lett.
- Journal Volume
- 53
- Journal Issue
- 6
- Series
- Phys. Rev. Lett.
- Journal Page Range
- 624-627
- ISSN
- 0031-9007
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 16019516
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANNIHILATION; ANTIPROTONS; COSMIC POSITRONS; COSMIC PROTONS; COSMIC RAY FLUX; COSMIC RAY PROPAGATION; COSMOLOGY; LEPTONS; MASS; POSTULATED PARTICLES; QUARKS; SUPERSYMMETRY; UNIVERSE
- Descriptors DEC
- ANTIBARYONS; ANTILEPTONS; ANTIMATTER; ANTINUCLEI; ANTINUCLEONS; ANTIPARTICLES; BARYONS; CATIONS; CHARGED PARTICLES; COSMIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; HADRONS; HYDROGEN IONS; HYDROGEN IONS 1 PLUS; INTERACTIONS; IONIZING RADIATIONS; IONS; MATTER; NUCLEI; NUCLEONS; PARTICLE INTERACTIONS; POSITRONS; PROTONS; RADIATION FLUX; RADIATIONS; SECONDARY COSMIC RADIATION; SYMMETRY