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b --> s$\gamma$ decay in supergravity grand unification and dark matter
An analysis of the b \rightarrow s\gamma is given in supergravity grand unification using the framework of the radiative breaking of the electro-weak symmetry under three separate sets of constraints:1) neutralino relic density does not overclose the universe,2)p-stability constraint, and 3) the com...
| Autores principales: | , |
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| Lenguaje: | eng |
| Publicado: |
1994
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1016/0370-2693(94)90550-9 http://cds.cern.ch/record/265337 |