CRESST-II: dark matter search with scintillating absorbers
In the CRESST-II experiment, scintillating CaWO4 crystals are used as absorbers for direct WIMP (weakly interacting massive particles) detection. Nuclear recoils can be discriminated against electron recoils by measuring phonons and scintillation light simultaneously. The absorber crystal and the si...
| Κύριοι συγγραφείς: | , , , , , , , , , , , , , , , , , , , , |
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| Μορφή: | Conference item |
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2005
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| _version_ | 1826268158885888000 |
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| author | Angloher, G Bucci, C Cozzini, C von Feilitzsch, F Frank, T Hauff, D Henry, S Jagemann, T Jochum, J Kraus, H Majorovits, B Ninkovic, J Petricca, F Probst, F Ramachers, Y Rau, W Seidel, W Stark, M Uchaikin, S Stodolsky, L Wulandari, H |
| author_facet | Angloher, G Bucci, C Cozzini, C von Feilitzsch, F Frank, T Hauff, D Henry, S Jagemann, T Jochum, J Kraus, H Majorovits, B Ninkovic, J Petricca, F Probst, F Ramachers, Y Rau, W Seidel, W Stark, M Uchaikin, S Stodolsky, L Wulandari, H |
| author_sort | Angloher, G |
| collection | OXFORD |
| description | In the CRESST-II experiment, scintillating CaWO4 crystals are used as absorbers for direct WIMP (weakly interacting massive particles) detection. Nuclear recoils can be discriminated against electron recoils by measuring phonons and scintillation light simultaneously. The absorber crystal and the silicon light detector are read out by tungsten superconducting phase transition thermometers (W-SPTs). Results on the sensitivity of the phonon and the light channel, radiopurity, the scintillation properties of CaWO4 and on the WIMP sensitivity are presented. |
| first_indexed | 2024-03-06T21:05:20Z |
| format | Conference item |
| id | oxford-uuid:3c3f14e7-df63-4317-ae50-bfb1e25527df |
| institution | University of Oxford |
| last_indexed | 2024-03-06T21:05:20Z |
| publishDate | 2005 |
| record_format | dspace |
| spelling | oxford-uuid:3c3f14e7-df63-4317-ae50-bfb1e25527df2022-03-26T14:12:30ZCRESST-II: dark matter search with scintillating absorbersConference itemhttp://purl.org/coar/resource_type/c_5794uuid:3c3f14e7-df63-4317-ae50-bfb1e25527dfSymplectic Elements at Oxford2005Angloher, GBucci, CCozzini, Cvon Feilitzsch, FFrank, THauff, DHenry, SJagemann, TJochum, JKraus, HMajorovits, BNinkovic, JPetricca, FProbst, FRamachers, YRau, WSeidel, WStark, MUchaikin, SStodolsky, LWulandari, HIn the CRESST-II experiment, scintillating CaWO4 crystals are used as absorbers for direct WIMP (weakly interacting massive particles) detection. Nuclear recoils can be discriminated against electron recoils by measuring phonons and scintillation light simultaneously. The absorber crystal and the silicon light detector are read out by tungsten superconducting phase transition thermometers (W-SPTs). Results on the sensitivity of the phonon and the light channel, radiopurity, the scintillation properties of CaWO4 and on the WIMP sensitivity are presented. |
| spellingShingle | Angloher, G Bucci, C Cozzini, C von Feilitzsch, F Frank, T Hauff, D Henry, S Jagemann, T Jochum, J Kraus, H Majorovits, B Ninkovic, J Petricca, F Probst, F Ramachers, Y Rau, W Seidel, W Stark, M Uchaikin, S Stodolsky, L Wulandari, H CRESST-II: dark matter search with scintillating absorbers |
| title | CRESST-II: dark matter search with scintillating absorbers |
| title_full | CRESST-II: dark matter search with scintillating absorbers |
| title_fullStr | CRESST-II: dark matter search with scintillating absorbers |
| title_full_unstemmed | CRESST-II: dark matter search with scintillating absorbers |
| title_short | CRESST-II: dark matter search with scintillating absorbers |
| title_sort | cresst ii dark matter search with scintillating absorbers |
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