First results from the CRESST-III low-mass dark matter program
| Autor: | CRESST Collaboration, Abdelhameed, A. H., Angloher, G., Bauer, P., Bento, A., Bertoldo, E., Bucci, C., Canonica, L., D'Addabbo, A., Defay, X., Di Lorenzo, S., Erb, A., Feilitzsch, F. v., Fichtinger, S., Iachellini, N. Ferreiro, Fuss, A., Gorla, P., Hauff, D., Jochum, J., Kinast, A., Kluck, H., Kraus, H., Langenkämper, A., Mancuso, M., Mokina, V., Mondragon, E., Münster, A., Olmi, M., Ortmann, T., Pagliarone, C., Pattavina, L., Petricca, F., Potzel, W., Pröbst, F., Reindl, F., Rothe, J., Schäffner, K., Schieck, J., Schipperges, V., Schmiedmayer, D., Schönert, S., Schwertner, C., Stahlberg, M., Stodolsky, L., Strandhagen, C., Strauss, R., Türkoglu, C., Usherov, I., Willers, M., Zema, V. |
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| Jazyk: | angličtina |
| Rok vydání: | 2019 |
| Předmět: |
Physics
Scintillation Cosmology and Nongalactic Astrophysics (astro-ph.CO) Dark Matter Cryogeny Calorimeter (particle physics) Phonon Physics::Instrumentation and Detectors Dark matter Detector Astrophysics::Instrumentation and Methods for Astrophysics FOS: Physical sciences Nuclear physics Recoil Particle Dark Matter Cryogeny Astrophysics - Instrumentation and Methods for Astrophysics Instrumentation and Methods for Astrophysics (astro-ph.IM) Light dark matter Astrophysics - Cosmology and Nongalactic Astrophysics |
| Zdroj: | Physical Review D. 100(10-15) |
| ISSN: | 2470-0029 2470-0010 |
| Popis: | The CRESST experiment is a direct dark matter search which aims to measure interactions of potential dark matter particles in an earth-bound detector. With the current stage, CRESST-III, we focus on a low energy threshold for increased sensitivity towards light dark matter particles. In this manuscript we describe the analysis of one detector operated in the first run of CRESST-III (05/2016-02/2018) achieving a nuclear recoil threshold of 30.1eV. This result was obtained with a 23.6g CaWO$_4$ crystal operated as a cryogenic scintillating calorimeter in the CRESST setup at the Laboratori Nazionali del Gran Sasso (LNGS). Both the primary phonon/heat signal and the simultaneously emitted scintillation light, which is absorbed in a separate silicon-on-sapphire light absorber, are measured with highly sensitive transition edge sensors operated at ~15mK. The unique combination of these sensors with the light element oxygen present in our target yields sensitivity to dark matter particle masses as low as 160MeV/c$^2$. 9 pages, 9 figures |
| Databáze: | OpenAIRE |
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