First Direct-Detection Results on Sub-GeV Dark Matter Using the SENSEI Detector at SNOLAB

We present the first results from a dark matter search using six Skipper-CCDs in the SENSEI detector operating at SNOLAB. We employ a bias-mitigation technique of hiding approximately 46% of our total data and aggressively mask images to remove backgrounds. Given a total exposure after masking of 100.72 gram-days from well-performing sensors, we observe 55 two-electron events, 4 three-electron events, and no events containing 4-10 electrons. The two-electron events are consistent with pileup from one-electron events. Among the 4 three-electron events, 2 appear in pixels that are likely impacted by detector defects, although not strongly enough to trigger our "hot-pixel" mask. We use these data to set world-leading constraints on sub-GeV dark matter interacting with electrons and nuclei.

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Publication Details

Journal
Physical Review Letters
Published
2025-01-09
DOI
https://doi.org/10.1103/physrevlett.134.011804
Citations
64
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
117.82

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article

First Direct-Detection Results on Sub-GeV Dark Matter Using the SENSEI Detector at SNOLAB

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Physical Review Letters
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article

First Direct-Detection Results on Sub-GeV Dark Matter Using the SENSEI Detector at SNOLAB

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article en
64 citations

Abstract

We present the first results from a dark matter search using six Skipper-CCDs in the SENSEI detector operating at SNOLAB. We employ a bias-mitigation technique of hiding approximately 46% of our total data and aggressively mask images to remove backgrounds. Given a total exposure after masking of 100.72 gram-days from well-performing sensors, we observe 55 two-electron events, 4 three-electron events, and no events containing 4-10 electrons. The two-electron events are consistent with pileup from one-electron events. Among the 4 three-electron events, 2 appear in pixels that are likely impacted by detector defects, although not strongly enough to trigger our "hot-pixel" mask. We use these data to set world-leading constraints on sub-GeV dark matter interacting with electrons and nuclei.

Physical Review LettersVol. 134(1)
Institut polytechnique de Grenoble (FR), Centre National de la Recherche Scientifique (FR), Fermi National Accelerator Laboratory (US), Lawrence Berkeley National Laboratory (US), Consejo Nacional de Investigaciones Científicas y Técnicas (AR), Stockholm University (SE), Tel Aviv University (IL), Universidad Nacional de Córdoba (AR), University of Oregon (US), Universidad de Buenos Aires (AR), University of Chicago (US), Institut National de Physique Nucléaire et de Physique des Particules (FR), Laboratoire de Physique Subatomique et de Cosmologie (FR), Snolab (CA), Instituto de Física de Buenos Aires (AR), Fundación Ciencias Exactas y Naturales (AR), Stony Brook University (US), Universidad Nacional Autónoma de México (MX), Université Grenoble Alpes (FR), University of California, Berkeley (US)
National Science Foundation, U.S. Department of Energy, Simons Foundation, Heising-Simons Foundation, Canada Foundation for Innovation, United States-Israel Binational Science Foundation, Israel Science Foundation, Azrieli Foundation, Office of Science, Horizon 2020 Framework Programme, European Research Council, High Energy Physics, Fermilab
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Openalex Percentile: Top 0%
Dark Matter and Cosmic Phenomena
117.82
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