Non--Baryonic Dark Matter
arXiv:astro-ph/9601188 · doi:10.1016/0920-5632(96)00199-5
Abstract
The best particle candidates for non--baryonic cold dark matter are reviewed, namely, neutralino, axion, axino and Majoron. These particles are considered in the context of cosmological models with the restrictions given by the observed mass spectrum of large scale structures, data on clusters of galaxies, age of the Universe etc.
Latex, 12 pages, espcrc2.sty, 6 figures included, appended as a uuencoded compressed tarred file. Invited talk at the TAUP95 workshop, presented by V. Berezinsky
References in corpus (12)
- Electroweak Symmetry Breaking with Non-Universal Scalar Soft Terms and Large Solutions
- Predictions in SU(5) Supergravity Grand Unification with Proton Stability and Relic Density Constraints
- Global String Radiation
- The KeV Majoron as Dark Matter Particle
- Planck Scale Effects on the Majoron
- Planck Scale Symmetry Breaking and Majoron Physics
- Damped Lyman Alpha Systems vs. Cold + Hot Dark Matter
- On the Neutralino as Dark Matter Candidate - II. Direct Detection
- Amount of Antiprotons in Cosmic Rays due to Halo Neutralino Annihilation
- Troubles with the Minimal SU(5) Supergravity Model
- Constraints on Majoron Models, Neutrino Masses and Baryogenesis
- Axion detection by ring lasers