Solar and Atmospheric Neutrinos: Background Sources for the Direct Dark Matter Searches

Physik-Department E15, Technische Universität München, D-85748 Garching, Germany
Astroparticle Physics (Impact Factor: 3.58). 03/2010; 34(2):90-96. DOI: 10.1016/j.astropartphys.2010.06.002
Source: arXiv


In experiments for direct dark matter searches, neutrinos coherently scattering off nuclei can produce similar events as Weakly Interacting Massive Particles (WIMPs). The calculated count rate for solar neutrinos in such experiments is a few events per ton-year. This count rate strongly depends on the nuclear recoil energy threshold achieved in the experiments for the WIMP search. We show that solar neutrinos can be a serious background source for direct dark matter search experiments using Ge, Ar, Xe and CaWO4 as target materials. To reach sensitivities better than ∼10−10 pb for the elastic WIMP nucleon spin-independent cross section in the zero-background limit, energy thresholds for nuclear recoils should be ≳2.05 keV for CaWO4, ≳4.91 keV for Ge, ≳2.89 keV for Xe, and ≳8.62 keV for Ar as target material. Next-generation experiments should not only strive for a reduction of the present energy thresholds but mainly focus on an increase of the target mass. Atmospheric neutrinos limit the achievable sensitivity for the background-free direct dark matter search to ≳10−12 pb.

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Available from: F. von Feilitzsch, Dec 20, 2013
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