Status and low background considerations for the CRESST dark matter search
We are preparing the CRESST experiment to search for dark matter WIMPs using cryogenic detectors with superconducting phase transition thermometers. In the first stage we plan to use four 250 g sapphire detectors with thresholds of 0.5 keV and resolutions of 0.2 keV at 1 keV. This will provide sensi...
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Conference item |
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1996
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| _version_ | 1826282091998871552 |
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| author | Buhler, M Zerle, L Probst, F Rulofs, A Schanda, U Seidel, W Absmaier, C Booth, N Bucci, C Colling, P Cooper, S vonFeilitzsch, F Ferger, P Forster, G Gabutti, A Hoss, C Hohne, J Igalson, J Kellner, E Koch, M Loidl, M Meier, O Nucciotti, A Nagel, U vanderPuute, M |
| author_facet | Buhler, M Zerle, L Probst, F Rulofs, A Schanda, U Seidel, W Absmaier, C Booth, N Bucci, C Colling, P Cooper, S vonFeilitzsch, F Ferger, P Forster, G Gabutti, A Hoss, C Hohne, J Igalson, J Kellner, E Koch, M Loidl, M Meier, O Nucciotti, A Nagel, U vanderPuute, M |
| author_sort | Buhler, M |
| collection | OXFORD |
| description | We are preparing the CRESST experiment to search for dark matter WIMPs using cryogenic detectors with superconducting phase transition thermometers. In the first stage we plan to use four 250 g sapphire detectors with thresholds of 0.5 keV and resolutions of 0.2 keV at 1 keV. This will provide sensitivity to WIMP masses below 10 GeV, and is thus complementary to other dark matter searches. |
| first_indexed | 2024-03-07T00:38:37Z |
| format | Conference item |
| id | oxford-uuid:8246178c-a2ed-4179-8142-f2d8228b2d2e |
| institution | University of Oxford |
| last_indexed | 2024-03-07T00:38:37Z |
| publishDate | 1996 |
| record_format | dspace |
| spelling | oxford-uuid:8246178c-a2ed-4179-8142-f2d8228b2d2e2022-03-26T21:36:17ZStatus and low background considerations for the CRESST dark matter searchConference itemhttp://purl.org/coar/resource_type/c_5794uuid:8246178c-a2ed-4179-8142-f2d8228b2d2eSymplectic Elements at Oxford1996Buhler, MZerle, LProbst, FRulofs, ASchanda, USeidel, WAbsmaier, CBooth, NBucci, CColling, PCooper, SvonFeilitzsch, FFerger, PForster, GGabutti, AHoss, CHohne, JIgalson, JKellner, EKoch, MLoidl, MMeier, ONucciotti, ANagel, UvanderPuute, MWe are preparing the CRESST experiment to search for dark matter WIMPs using cryogenic detectors with superconducting phase transition thermometers. In the first stage we plan to use four 250 g sapphire detectors with thresholds of 0.5 keV and resolutions of 0.2 keV at 1 keV. This will provide sensitivity to WIMP masses below 10 GeV, and is thus complementary to other dark matter searches. |
| spellingShingle | Buhler, M Zerle, L Probst, F Rulofs, A Schanda, U Seidel, W Absmaier, C Booth, N Bucci, C Colling, P Cooper, S vonFeilitzsch, F Ferger, P Forster, G Gabutti, A Hoss, C Hohne, J Igalson, J Kellner, E Koch, M Loidl, M Meier, O Nucciotti, A Nagel, U vanderPuute, M Status and low background considerations for the CRESST dark matter search |
| title | Status and low background considerations for the CRESST dark matter search |
| title_full | Status and low background considerations for the CRESST dark matter search |
| title_fullStr | Status and low background considerations for the CRESST dark matter search |
| title_full_unstemmed | Status and low background considerations for the CRESST dark matter search |
| title_short | Status and low background considerations for the CRESST dark matter search |
| title_sort | status and low background considerations for the cresst dark matter search |
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