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Hot QCD and warm dark matter

Name: Hot QCD and warm dark matter
Creator: Laine, Mikko
Keywords: High Energy Physics - Lattice, High Energy Physics - Lattice (hep-lat), 0103 physical sciences, FOS: Physical sciences, 01 natural sciences, 7. Clean energy

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type , Conference object 18 Dec 2006Embargo end date: 01 Jan 2006 Germany Publisher:Sissa MedialabJournal:Proceedings of XXIVth International Symposium on Lattice Field Theory — PoS(LAT2006)

Authors: Laine, Mikko;

doi: 10.22323/1.032.0014 , 10.48550/arxiv.hep-lat/0612023

arXiv: http://arxiv.org/abs/hep-lat/0612023

Hot QCD and warm dark matter

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Abstract

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.

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

Country

Germany

Related Organizations

Bielefeld University
Germany

Keywords

High Energy Physics - Lattice, High Energy Physics - Lattice (hep-lat), FOS: Physical sciences

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	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average