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- W2180182406 abstract "If the energy density of the Universe before nucleosynthesis is dominated by a scalar field $ensuremath{phi}$ that decays and reheats the plasma to a temperature ${T}_{mathrm{RH}}$ 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: ${T}_{mathrm{RH}}$, and the number of neutralinos produced per $ensuremath{phi}$ decay per unit mass of the $ensuremath{phi}$ 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." @default.
- W2180182406 created "2016-06-24" @default.
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- W2180182406 date "2006-10-18" @default.
- W2180182406 modified "2023-09-26" @default.
- W2180182406 title "Effect of a late decaying scalar on the neutralino relic density" @default.
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- W2180182406 doi "https://doi.org/10.1103/physrevd.74.083514" @default.
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