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The effect of a late decaying scalar on the neutralino relic density

Graciela Gelmini·Paolo Gondolo·Adrian Soldatenko·Carlos E. Yaguna
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Abstract

If the energy density of the Universe before nucleosynthesis is dominated by a scalar field phi that decays and reheats the plasma to a temperature T_{RH} smaller than the standard neutralino freeze out temperature, the neutralino relic density differs from its standard value. In this case, the relic density depends on two additional parameters: T_{RH}, and the number of neutralinos produced per phi decay per unit mass of the phi field. In this paper, we numerically study the neutralino relic density as a function of these reheating parameters within minimal supersymmetric standard models and show that the dark matter constraint can almost always be satisfied.

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Graciela Gelmini, Paolo Gondolo, Adrian Soldatenko, Carlos E. Yaguna. 2006-05-01. The effect of a late decaying scalar on the neutralino relic density. https://doi.org/10.1103/physrevd.74.083514

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