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Home Search Quick Search Advanced Fulltext Browse Collections Persons My eDoc Session History Login Name: Password: Documentation Help Support Wiki Direct access to document ID:	Institute: MPI für Physik     Collection: YB 2016     Display Documents ID: 716341.0, MPI für Physik / YB 2016 Impact of Coherent Neutrino Nucleus Scattering on Direct Dark Matter Searches based on CaWO$_4$ Crystals Authors: Gütlein, A.; Angloher, G.; Bento, A.; Bucci, C.; Canonica, L.; Erb, A.; Feilitzsch, F. v.; Ferreiro Iachellini, N.; Gorla, P.; Hauff, D.; Jochum, J.; Kiefer, M.; Kluck, H.; Kraus, H.; Lanfranchi, J. -C.; Loebell, J.; Münster, A.; Petricca, F.; Potzel, W.; Pröbst, F.; Reindl, F.; Roth, S.; Rottler, K.; Sailer, C.; Schäffner, K.; Schieck, J.; Schönert, S.; Seidel, W.; Sivers, M. v.; Stodolsky, L.; Strandhagen, C.; Strauss, R.; Tanzke, A.; Uffinger, M.; Ulrich, A.; Usherov, I.; Wawoczny, S.; Willers, M.; Wüstrich, M.; Zöller, A. Date of Publication (YYYY-MM-DD): 2015 Title of Journal: Astroparticle Physics Journal Abbrev.: Astropart.Phys. Issue / Number: 69 Start Page: 44 Audience: Not Specified Intended Educational Use: No Abstract / Description: 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. Classification / Thesaurus: CRESST Comment of the Author/Creator: submitted to Astorparticle Physics External Publication Status: published Document Type: Article Communicated by: MPI für Physik Affiliations: MPI für Physik Identifiers: LOCALID:MPP-2015-380 URL:http://inspirehep.net/search?p=find+eprint+1408.23... URL:http://arXiv.org/abs/arxiv:1408.2357 URL:https://publications.mppmu.mpg.de/?action=search&m... Full Text: You have privileges to view the following file(s): arxiv:1408.2357.pdf   Uploading file not finished... The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.