The CRESST dark matter search
We present first competitive results on WIMP dark matter using the phonon-light-detection technique. A particularly strong limit for WIMPs with coherent scattering results from selecting a region of the phonon-light plane corresponding to tungsten recoils. The observed count rate in the neutron band...
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Conference item |
| Published: |
2005
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| _version_ | 1826271063100620800 |
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| author | Majorovits, B Cozzini, C Henry, S Kraus, H Mikhailik, V Tolhurst, A Wahl, D Ramachers, Y Angloher, G Christ, P Hauff, D Ninkovic, J Petricca, F Probst, F Seidel, W Stodolsky, L Feilitzsch, F Jagemann, T Potzel, W Razeti, M Rau, W Stark, M Westphal, W Wulandari, H Jochum, J |
| author_facet | Majorovits, B Cozzini, C Henry, S Kraus, H Mikhailik, V Tolhurst, A Wahl, D Ramachers, Y Angloher, G Christ, P Hauff, D Ninkovic, J Petricca, F Probst, F Seidel, W Stodolsky, L Feilitzsch, F Jagemann, T Potzel, W Razeti, M Rau, W Stark, M Westphal, W Wulandari, H Jochum, J |
| author_sort | Majorovits, B |
| collection | OXFORD |
| description | We present first competitive results on WIMP dark matter using the phonon-light-detection technique. A particularly strong limit for WIMPs with coherent scattering results from selecting a region of the phonon-light plane corresponding to tungsten recoils. The observed count rate in the neutron band is compatible with the rate expected from neutron background. CRESST is presently being upgraded with a 66 channel SQUID readout system, a neutron shield and a muon veto system. This results in a significant improvement in sensitivity. |
| first_indexed | 2024-03-06T21:50:44Z |
| format | Conference item |
| id | oxford-uuid:4b27e594-ebeb-49ea-ac2c-3e1b0bd942ae |
| institution | University of Oxford |
| last_indexed | 2024-03-06T21:50:44Z |
| publishDate | 2005 |
| record_format | dspace |
| spelling | oxford-uuid:4b27e594-ebeb-49ea-ac2c-3e1b0bd942ae2022-03-26T15:42:01ZThe CRESST dark matter searchConference itemhttp://purl.org/coar/resource_type/c_5794uuid:4b27e594-ebeb-49ea-ac2c-3e1b0bd942aeSymplectic Elements at Oxford2005Majorovits, BCozzini, CHenry, SKraus, HMikhailik, VTolhurst, AWahl, DRamachers, YAngloher, GChrist, PHauff, DNinkovic, JPetricca, FProbst, FSeidel, WStodolsky, LFeilitzsch, FJagemann, TPotzel, WRazeti, MRau, WStark, MWestphal, WWulandari, HJochum, JWe present first competitive results on WIMP dark matter using the phonon-light-detection technique. A particularly strong limit for WIMPs with coherent scattering results from selecting a region of the phonon-light plane corresponding to tungsten recoils. The observed count rate in the neutron band is compatible with the rate expected from neutron background. CRESST is presently being upgraded with a 66 channel SQUID readout system, a neutron shield and a muon veto system. This results in a significant improvement in sensitivity. |
| spellingShingle | Majorovits, B Cozzini, C Henry, S Kraus, H Mikhailik, V Tolhurst, A Wahl, D Ramachers, Y Angloher, G Christ, P Hauff, D Ninkovic, J Petricca, F Probst, F Seidel, W Stodolsky, L Feilitzsch, F Jagemann, T Potzel, W Razeti, M Rau, W Stark, M Westphal, W Wulandari, H Jochum, J The CRESST dark matter search |
| title | The CRESST dark matter search |
| title_full | The CRESST dark matter search |
| title_fullStr | The CRESST dark matter search |
| title_full_unstemmed | The CRESST dark matter search |
| title_short | The CRESST dark matter search |
| title_sort | cresst dark matter search |
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