CRESST: First results with the phonon-light technique
We present first significant limits on WIMP dark matter by the phonon-light technique, where combined phonon and light signals from a scintillating cryogenic detector are used to suppress the non-nuclear recoil background. The performance of the detectors developed for the second phase of the CRESST...
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Conference item |
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2006
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| _version_ | 1826303331000123392 |
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| author | Petricca, F Angloher, G Bucci, C Christ, P Cozzini, C von Fellitzsch, F Hauff, D Henry, S Jagemann, T Jochum, J Kraus, H Majorovits, B Ninkovic, J Potzel, W Proebst, F Ramachers, Y Rau, W Seidel, W Stark, M Stodolsky, L Westphal, W Wulandari, H |
| author_facet | Petricca, F Angloher, G Bucci, C Christ, P Cozzini, C von Fellitzsch, F Hauff, D Henry, S Jagemann, T Jochum, J Kraus, H Majorovits, B Ninkovic, J Potzel, W Proebst, F Ramachers, Y Rau, W Seidel, W Stark, M Stodolsky, L Westphal, W Wulandari, H |
| author_sort | Petricca, F |
| collection | OXFORD |
| description | We present first significant limits on WIMP dark matter by the phonon-light technique, where combined phonon and light signals from a scintillating cryogenic detector are used to suppress the non-nuclear recoil background. The performance of the detectors developed for the second phase of the CRESST experiment will be discussed and data collected with two prototype modules in a short run, corresponding to a net exposure of 20.5 kg days, will be presented. (c) 2005 Elsevier B.V. All rights reserved. |
| first_indexed | 2024-03-07T06:01:03Z |
| format | Conference item |
| id | oxford-uuid:ec327ebf-3d20-4600-bf5d-af8607c0aa3b |
| institution | University of Oxford |
| last_indexed | 2024-03-07T06:01:03Z |
| publishDate | 2006 |
| record_format | dspace |
| spelling | oxford-uuid:ec327ebf-3d20-4600-bf5d-af8607c0aa3b2022-03-27T11:15:43ZCRESST: First results with the phonon-light techniqueConference itemhttp://purl.org/coar/resource_type/c_5794uuid:ec327ebf-3d20-4600-bf5d-af8607c0aa3bSymplectic Elements at Oxford2006Petricca, FAngloher, GBucci, CChrist, PCozzini, Cvon Fellitzsch, FHauff, DHenry, SJagemann, TJochum, JKraus, HMajorovits, BNinkovic, JPotzel, WProebst, FRamachers, YRau, WSeidel, WStark, MStodolsky, LWestphal, WWulandari, HWe present first significant limits on WIMP dark matter by the phonon-light technique, where combined phonon and light signals from a scintillating cryogenic detector are used to suppress the non-nuclear recoil background. The performance of the detectors developed for the second phase of the CRESST experiment will be discussed and data collected with two prototype modules in a short run, corresponding to a net exposure of 20.5 kg days, will be presented. (c) 2005 Elsevier B.V. All rights reserved. |
| spellingShingle | Petricca, F Angloher, G Bucci, C Christ, P Cozzini, C von Fellitzsch, F Hauff, D Henry, S Jagemann, T Jochum, J Kraus, H Majorovits, B Ninkovic, J Potzel, W Proebst, F Ramachers, Y Rau, W Seidel, W Stark, M Stodolsky, L Westphal, W Wulandari, H CRESST: First results with the phonon-light technique |
| title | CRESST: First results with the phonon-light technique |
| title_full | CRESST: First results with the phonon-light technique |
| title_fullStr | CRESST: First results with the phonon-light technique |
| title_full_unstemmed | CRESST: First results with the phonon-light technique |
| title_short | CRESST: First results with the phonon-light technique |
| title_sort | cresst first results with the phonon light technique |
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