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, L., Pepe, C., Sarnoff, I., Ibrayev, T., Oikonomou, P., Knyazev, A., Monticone, E., Garrone, H., Alder, F., Fawwaz, O., Millar, A.J., Morå, K.D., Shams, H., Arneodo, F., Rajteri, M.. - 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.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11696/83939
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