1. Impact of coherent neutrino nucleus scattering on direct dark matter searches based on CaWO 4 crystals
- Author
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M. Willers, R. Strauss, D. Hauff, Franz von Feilitzsch, A. Gütlein, F. Pröbst, J. Loebell, W. Seidel, A. Münster, G. Angloher, Andreas Erb, N. Ferreiro Iachellini, A. Tanzke, A.C.S.S.M. Bento, F. Petricca, Leo Stodolsky, Lucia Canonica, I. Usherov, M. Wüstrich, C. Bucci, F. Reindl, A. Zöller, S. Wawoczny, Jochen Schieck, M. Uffinger, M. v. Sivers, M. Kiefer, W. Potzel, S. Roth, J.-C. Lanfranchi, C. Sailer, S. Schönert, P. Gorla, K. Rottler, C. Strandhagen, A. Ulrich, H. Kluck, K. Schäffner, J. Jochum, and H. Kraus
- Subjects
Physics ,Particle physics ,Physics - Instrumentation and Detectors ,Physics::Instrumentation and Detectors ,Scattering ,Solar neutrino ,Dark matter ,FOS: Physical sciences ,Astronomy and Astrophysics ,Instrumentation and Detectors (physics.ins-det) ,Solar neutrino problem ,Nuclear physics ,High Energy Physics - Phenomenology ,High Energy Physics - Phenomenology (hep-ph) ,Neutrino detector ,Measurements of neutrino speed ,High Energy Physics::Experiment ,Neutrino ,Neutrino oscillation - Abstract
Atmospheric and solar neutrinos scattering coherently off target nuclei will be an important background source for the next generation of direct dark matter searches. In this work we focus on calcium tungstate as target material. For comparison with existing works we calculate the neutrino floor indicating which sensitivities can be reached before the neutrino background appears. In addition, we investigate the sensitivities of future direct dark matter searches using CRESST-II like detectors. Extending previous works we take into account achievable energy resolutions and thresholds as well as beta and gamma backgrounds for this investigation. We show that an exploration of WIMP-nucleon cross sections below the neutrino floor is possible for exposures of $\gtrsim10$ kg-years or higher. In the third part we show that a first detection of coherent neutrino nucleus scattering of atmospheric and solar neutrinos using the same detectors and the backgrounds is feasible for exposures of $\gtrsim50$ kg-years., submitted to Astorparticle Physics
- Published
- 2015
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