Detector Development for the CRESST Experiment
Recently low-mass dark matter direct searches have been hindered by a low-energy background, drastically reducing the physics reach of the experiments. In the CRESST-III experiment, this signal is characterised by a significant increase of events below 200 eV. As the origin of this background is sti...
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
Springer
2024
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| _version_ | 1826313715031474176 |
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| author | Angloher, G Banik, S Benato, G Bento, A Bertolini, A Breier, R Bucci, C Burkhart, J Canonica, L D’Addabbo, A Di Lorenzo, S Einfalt, L Erb, A Feilitzsch, FV Fichtinger, S Fuchs, D Garai, A Ghete, VM Gorla, P Guillaumon, PV Gupta, S Hauff, D Ješkovský, M Jochum, J Kraus, H |
| author_facet | Angloher, G Banik, S Benato, G Bento, A Bertolini, A Breier, R Bucci, C Burkhart, J Canonica, L D’Addabbo, A Di Lorenzo, S Einfalt, L Erb, A Feilitzsch, FV Fichtinger, S Fuchs, D Garai, A Ghete, VM Gorla, P Guillaumon, PV Gupta, S Hauff, D Ješkovský, M Jochum, J Kraus, H |
| author_sort | Angloher, G |
| collection | OXFORD |
| description | Recently low-mass dark matter direct searches have been hindered by a low-energy background, drastically reducing the physics reach of the experiments. In the CRESST-III experiment, this signal is characterised by a significant increase of events below 200 eV. As the origin of this background is still unknown, it became necessary to develop new detector designs to reach a better understanding of the observations. Within the CRESST collaboration, three new different detector layouts have been developed, and they are presented in this contribution. |
| first_indexed | 2024-09-25T04:19:20Z |
| format | Journal article |
| id | oxford-uuid:b3630f90-f0f9-4435-9db5-5f63627094fe |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-09-25T04:19:20Z |
| publishDate | 2024 |
| publisher | Springer |
| record_format | dspace |
| spelling | oxford-uuid:b3630f90-f0f9-4435-9db5-5f63627094fe2024-07-27T19:38:43ZDetector Development for the CRESST ExperimentJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:b3630f90-f0f9-4435-9db5-5f63627094feEnglishJisc Publications RouterSpringer2024Angloher, GBanik, SBenato, GBento, ABertolini, ABreier, RBucci, CBurkhart, JCanonica, LD’Addabbo, ADi Lorenzo, SEinfalt, LErb, AFeilitzsch, FVFichtinger, SFuchs, DGarai, AGhete, VMGorla, PGuillaumon, PVGupta, SHauff, DJeškovský, MJochum, JKraus, HRecently low-mass dark matter direct searches have been hindered by a low-energy background, drastically reducing the physics reach of the experiments. In the CRESST-III experiment, this signal is characterised by a significant increase of events below 200 eV. As the origin of this background is still unknown, it became necessary to develop new detector designs to reach a better understanding of the observations. Within the CRESST collaboration, three new different detector layouts have been developed, and they are presented in this contribution. |
| spellingShingle | Angloher, G Banik, S Benato, G Bento, A Bertolini, A Breier, R Bucci, C Burkhart, J Canonica, L D’Addabbo, A Di Lorenzo, S Einfalt, L Erb, A Feilitzsch, FV Fichtinger, S Fuchs, D Garai, A Ghete, VM Gorla, P Guillaumon, PV Gupta, S Hauff, D Ješkovský, M Jochum, J Kraus, H Detector Development for the CRESST Experiment |
| title | Detector Development for the CRESST Experiment |
| title_full | Detector Development for the CRESST Experiment |
| title_fullStr | Detector Development for the CRESST Experiment |
| title_full_unstemmed | Detector Development for the CRESST Experiment |
| title_short | Detector Development for the CRESST Experiment |
| title_sort | detector development for the cresst experiment |
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