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arXiv · 0809.1982

Quintessential Kination and Thermal Production of SUSY e-WIMPs

M. E. Gomez·S. Lola·C. Pallis·J. Rodriguez-Quintero
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Abstract

The impact of a kination-dominated phase generated by a quintessential exponential model on the thermal abundance of Supersymmetric (SUSY) extremely Weekly Interacting Massive Particles (e-WIMPs) is investigated. For values of the quintessential energy-density parameter on the eve of nucleosynthesis close to its upper bound, we find that: (i) the gravitino constraint is totally evaded for unstable gravitinos; (ii) the thermal abundance of stable gravitinos is not sufficient to account for the cold dark matter of the universe; (iii) the thermal abundance of axinos can satisfy the cold dark matter constraint for values of the initial (``reheating'') temperature well above those required in the standard cosmology.

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M. E. Gomez, S. Lola, C. Pallis, J. Rodriguez-Quintero. 2008-09-11. Quintessential Kination and Thermal Production of SUSY e-WIMPs. https://doi.org/10.1063/1.3131490

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