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

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arxiv 2212.12513 v2 pith:CJCURGLQ submitted 2022-12-23 astro-ph.CO

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

classification astro-ph.CO
keywords darkenergymattercresst-iiiparticlesresultssilicontext
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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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  1. First Limits on Light Dark Matter Interactions in a Low Threshold Two Channel Athermal Phonon Detector from the TESSERACT Collaboration

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    A 0.233 g silicon athermal phonon detector with 361.5 MeV/c² rms resolution sets the strongest direct-detection limits on dark matter-nucleon cross sections for masses 44–87 MeV/c² after 12 hours of exposure.