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Supersymmetric Dark Matter with a Cosmological Constant
Recent measurements of cosmological parameters from the microwave background radiation, type Ia supernovae, and the age of globular clusters help determine the relic matter density in the universe. It is first shown with mild cosmological assumptions that the relic matter density satisfies $\Omega_M...
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Lenguaje: | eng |
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1998
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Acceso en línea: | https://dx.doi.org/10.1016/S0370-2693(98)01327-6 http://cds.cern.ch/record/366088 |