Superconducting transition-edge sensors (TESs) are a type of quantum sensor known for their high single-photon detection efficiency and low background. This makes TESs ideal for particle-physics experiments searching for rare events. In this work, we present a comprehensive characterization of the background in optical TESs, distinguishing three types of events: electrical-noise, high-energy, and photonlike events. We introduce computational methods to automate the classification of events. We experimentally verify and simulate the source of the high-energy events. We also isolate the photonlike events, the expected signal in dielectric haloscopes searching for dark-matter dark photons, and achieve a photonlike dark-count rate of 3.6x10-4 - 4 in the 0.8-3.2 eV energy range.
Dark counts in optical superconducting transition-edge sensors for rare-event searches / Manenti, Laura; Pepe, Carlo; Sarnoff, Isaac; Ibrayev, Tengiz; Oikonomou, Panagiotis; Knyazev, Artem; Monticone, Eugenio; Garrone, Hobey; Alder, Fiona; Fawwaz, Osama; Millar, Alexander J.; Morå, Knut Dundas; Shams, Hamad; Arneodo, Francesco; Rajteri, Mauro. - In: PHYSICAL REVIEW APPLIED. - ISSN 2331-7019. - 22:2(2024). [10.1103/physrevapplied.22.024051]
Dark counts in optical superconducting transition-edge sensors for rare-event searches
Pepe, Carlo;Monticone, Eugenio;Garrone, Hobey;Rajteri, Mauro
2024
Abstract
Superconducting transition-edge sensors (TESs) are a type of quantum sensor known for their high single-photon detection efficiency and low background. This makes TESs ideal for particle-physics experiments searching for rare events. In this work, we present a comprehensive characterization of the background in optical TESs, distinguishing three types of events: electrical-noise, high-energy, and photonlike events. We introduce computational methods to automate the classification of events. We experimentally verify and simulate the source of the high-energy events. We also isolate the photonlike events, the expected signal in dielectric haloscopes searching for dark-matter dark photons, and achieve a photonlike dark-count rate of 3.6x10-4 - 4 in the 0.8-3.2 eV energy range.File | Dimensione | Formato | |
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