PIRSA:12040057  ( MP4 Medium Res , MP4 Low Res , MP3 , PDF ) Which Format?
UV Sensitivity of Dark Matter
Speaker(s): Scott Watson
Abstract: In this talk I will present evidence that accounting for the presence of hierarchies in string compactifications naturally leads to a UV sensitivity of dark matter in contrast to what is usually assumed. In particular, we will see that the existence of cosmological moduli may lead to a non-thermal history for the early universe and modifications in the primordial production of dark matter. If such a history were realized it would not only require probing new regions in dark matter searches, but also imply that a detection of dark matter would provide a direct probe on the early universe and the UV -- contrary to the thermal WIMP case. Regardless of the history of the early universe I will argue that if current string constructions are representative of more general models then all weak-scale dark matter would indeed be UV sensitive and would be a new prediction of string theory - falsifiable by experiment.
Date: 17/04/2012 - 11:00 am
Tech Note: First 20 minutes not captured
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