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Results on sub-GeV Dark Matter from a 10 eV Threshold CRESST-III Silicon Detector

Authors :
CRESST Collaboration
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, F. v.
Iachellini, N. Ferreiro
Fichtinger, S.
Fuchs, D.
Fuss, A.
Garai, A.
Ghete, V. M.
Gerster, S.
Gorla, P.
Guillaumon, P. V.
Gupta, S.
Hauff, D.
Ješkovský, M.
Jochum, J.
Kaznacheeva, M.
Kinast, A.
Kluck, H.
Kraus, H.
Langenkämper, A.
Mancuso, M.
Marini, L.
Meyer, L.
Mokina, V.
Nilima, A.
Olmi, M.
Ortmann, T.
Pagliarone, C.
Pattavina, L.
Petricca, F.
Potzel, W.
Povinec, P.
Pröbst, F.
Pucci, F.
Reindl, F.
Rothe, J.
Schäffner, K.
Schieck, J.
Schmiedmayer, D.
Schönert, S.
Schwertner, C.
Stahlberg, M.
Stodolsky, L.
Strandhagen, C.
Strauss, R.
Usherov, I.
Wagner, F.
Willers, M.
Zema, V.
Source :
Phys. Rev. D 107, 122003 (2023)
Publication Year :
2022

Abstract

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.<br />Comment: 8 pages, 5 figures; precised the position of the calibration source in Fig. 1; extended the discussion about the observed energy spectrum; added the DM limit curve to ancillary files. Published in Phys. Rev. D

Details

Database :
arXiv
Journal :
Phys. Rev. D 107, 122003 (2023)
Publication Type :
Report
Accession number :
edsarx.2212.12513
Document Type :
Working Paper
Full Text :
https://doi.org/10.1103/PhysRevD.107.122003