摘要: We present limits on the spin-independent interaction cross section of dark
matter particles with silicon nuclei, derived from data taken with a cryogenic
calorimeter with 0.35 g target mass operated in the CRESST-III experiment. A
baseline nuclear recoil energy resolution of $(1.36\pm 0.05)$ eV$_{\text{nr}}$,
currently the lowest reported for macroscopic particle detectors, and a
corresponding energy threshold of $(10.0\pm 0.2)$ eV$_{\text{nr}}$ have been
achieved, improving the sensitivity to light dark matter particles with masses
below 160 MeV/c$^2$ by a factor of up to 20 compared to previous results. We
characterize the observed low energy excess, and we exclude noise triggers and
radioactive contaminations on the crystal surfaces as dominant contributions.
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分类:
天文学
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天文学
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引用:
ChinaXiv:202303.03593
(或此版本
ChinaXiv:202303.03593V1)
DOI:10.12074/202303.03593V1
CSTR:32003.36.ChinaXiv.202303.03593.V1
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科创链TXID:
4eaf0ed4-85c9-46fa-a710-2a8881ef79b6
- 推荐引用方式:
CRESST Collaboration,G. Angloher,S. Banik,G. Benato,A. Bento,A. Bertolini,R. Breier,C. Bucci,J. Burkhart,L. Canonica,A. D'Addabbo,S. Di Lorenzo,L. Einfalt,A. Erb,F. v. Feilitzsch,N. Ferreiro Iachellini,S. Fichtinger,D. Fuchs,A. Fuss,A. Garai,V. M. Ghete,S. Gerster,P. Gorla,P. V. Guillaumon,S. Gupta,D. Hauff,M. Ješkovský,J. Jochum,M. Kaznacheeva,A. Kinast,H. Kluck,H. Kraus,A. Langenkämper,M. Mancuso,L. Marini,L. Meyer,V. Mokina,A. Nilima,M. Olmi,T. Ortmann,C. Pagliarone,L. Pattavina,F. Petricca,W. Potzel,P. Povinec,F. Pröbst,F. Pucci,F. Reindl,J. Rothe,K. Schäffner,J. Schieck,D. Schmiedmayer,S. Schönert,C. Schwertner,M. Stahlberg,L. Stodolsky,C. Strandhagen,R. Strauss,I. Usherov,F. Wagner,M. Willers,V. Zema.Results on sub-GeV Dark Matter from a 10 eV Threshold CRESST-III Silicon
Detector.null.[ChinaXiv:202303.03593V1]
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