2021
DOI: 10.1103/physrevlett.127.081802
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Constraints on Lightly Ionizing Particles from CDMSlite

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Cited by 6 publications
(4 citation statements)
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“…In recent years, cryogenic bolometers have established themselves as a powerful technology in rare event searches for 0νββ [9,[11][12][13][14][15][16], direct Dark Matter detection [17][18][19], and more [20][21][22][23][24]. Such detectors operate at milli-kelvin temperatures and measure energy deposition events by converting phonons into a temperature increase within a sensitive thermistor.…”
Section: Introductionmentioning
confidence: 99%
“…In recent years, cryogenic bolometers have established themselves as a powerful technology in rare event searches for 0νββ [9,[11][12][13][14][15][16], direct Dark Matter detection [17][18][19], and more [20][21][22][23][24]. Such detectors operate at milli-kelvin temperatures and measure energy deposition events by converting phonons into a temperature increase within a sensitive thermistor.…”
Section: Introductionmentioning
confidence: 99%
“…Despite their smaller exposures in terms of area-steradian coverage compared to traditional large-volume liquid or plastic scintillators or gaseous trackers, such contemporary solidstate detectors benefit from high energy resolution and low 𝑑𝐸/𝑑𝑥 thresholds. Combined with their typical placement in deep underground labs, this can result in competitive sensitivity to exotic tracklike phenomena including multiply-interacting dark matter [1] and lightly-ionizing particles (LIPs) [2,3]. Conversely, as the background requirements of these rare-event searches become increasingly stringent, it is valuable to have a precise in situ characterization of cosmogenic backgrounds such as muon-induced spallation products [4][5][6].…”
Section: Introductionmentioning
confidence: 99%
“…Despite their smaller exposures in terms of area-steradian coverage compared to traditional large-volume liquid or plastic scintillators or gaseous trackers, such contemporary solid-state detectors benefit from high energy resolution and low 𝑑𝐸/𝑑𝑥 thresholds. Combined with their typical placement in deep underground labs, this can result in competitive sensitivity to exotic track-like phenomena including multiply-interacting dark matter [1] and lightly-ionizing particles (LIPs) [2,3]. Conversely, as the background requirements of these rare-event searches become increasingly stringent, it is valuable to have a precise in situ characterization of cosmogenic backgrounds such as muon-induced spallation products [4][5][6].…”
Section: Introductionmentioning
confidence: 99%