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

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\(...

Full description

Saved in:
Bibliographic Details
Published inarXiv.org
Main Authors Collaboration, CRESST, Angloher, G, Banik, S, Benato, G, Bento, A, Bertolini, A, Breier, R, Bucci, C, Burkhart, J, Canonica, L, D'Addabbo, A, S Di Lorenzo, Einfalt, L, Erb, A, Feilitzsch, F v, N Ferreiro Iachellini, 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
Format Paper Journal Article
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 23.06.2023
Subjects
Online AccessGet full text

Cover

Loading…
More Information
Summary: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.
ISSN:2331-8422
DOI:10.48550/arxiv.2212.12513