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2013

Non-thermal Dark Matter in String Compactifications

Allahverdi, Rouzbeh, Cicoli, Michele, Dutta, Bhaskar et al.

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Non-thermal cosmological histories are capable of greatly increasing the available parameter space of different particle physics dark matter (DM) models and are well-motivated by the ubiquity of late-decaying gravitationally coupled scalars in UV theories like string theory.

A non-thermal DM model is presented in the context of LARGE Volume Scenarios in type IIB string theory.
The model is capable of addressing both the moduli-induced gravitino problem as well as the problem of overproduction of axionic dark radiation and/or DM.
We show that the right abundance of neutralino DM can be obtained in both thermal under and overproduction cases for DM masses between O(GeV) to O(TeV).

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