Hot QCD and warm dark matter

Details Hot QCD and warm dark matter Hot QCD and warm dark matter

2006-12-20

arxiv.org/abs/hep-lat/0612023v1

PoSLAT2006:014,2006

Physics

High Energy Physics

High Energy Physics - Lattice

15 pages. Updated version of plenary talk at International Symposium on Lattice Field Theory, July 23-28, 2006, Tucson, Arizon

Scientific paper

One of the possible explanations for the dark matter needed in the standard cosmological model is so-called warm dark matter, in the form of right-handed ("sterile") neutrinos with a mass in the keV range. I describe how various properties of QCD at temperatures of a few hundred MeV play an important role in the theoretical computations that are needed for consolidating or falsifying this scenario. In particular the points where lattice QCD could help are underlined.

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