2021
DOI: 10.1016/j.scib.2021.02.024
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Mid-infrared single photon detector with superconductor Mo0.8Si0.2 nanowire

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Cited by 38 publications
(14 citation statements)
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“…SNSPDs were previously shown to achieve high detection efficiencies (>90%) in the near-infrared range (780–1000 nm) , and the telecom bands (1300–1600 nm). To achieve a high detection efficiency in the 1300–2000 nm range, several factors were optimized: the NbTiN superconducting film composition, the geometry of the superconducting nanowires (as shown in Figure a), and the optical cavity formed by a Au mirror and SiO 2 spacer underneath the superconducting film. Although mid-infrared detectors have been demonstrated for light with wavelengths ranging from 1 to 5 μm , or even 10 μm, these demonstrations either showed a saturated internal efficiency or demonstrated a limited detection efficiency . Moreover, the materials used in most of these demonstrations (apart from) required operation below the base temperature of conventional Gifford–McMahon cryo-coolers, making the development of a compact microscopy system much more difficult.…”
Section: Resultsmentioning
confidence: 99%
“…SNSPDs were previously shown to achieve high detection efficiencies (>90%) in the near-infrared range (780–1000 nm) , and the telecom bands (1300–1600 nm). To achieve a high detection efficiency in the 1300–2000 nm range, several factors were optimized: the NbTiN superconducting film composition, the geometry of the superconducting nanowires (as shown in Figure a), and the optical cavity formed by a Au mirror and SiO 2 spacer underneath the superconducting film. Although mid-infrared detectors have been demonstrated for light with wavelengths ranging from 1 to 5 μm , or even 10 μm, these demonstrations either showed a saturated internal efficiency or demonstrated a limited detection efficiency . Moreover, the materials used in most of these demonstrations (apart from) required operation below the base temperature of conventional Gifford–McMahon cryo-coolers, making the development of a compact microscopy system much more difficult.…”
Section: Resultsmentioning
confidence: 99%
“…These measures could equally apply to SatQKD but there is also the possibility of utilising wavelengths with better penetration of partially obscured skies, particularly in the mid to long infrared region of the spectrum [294]. This requires the development of new sources and detectors but some progress has been made in this direction [295][296][297].…”
Section: Impact Of the Atmosphere: Turbulence Noise And Weathermentioning
confidence: 99%
“…[52][53][54]). These devices are sensitive to the deposit of extremely small amounts of energy, with proven sub-eV thresholds and low dark count rates [24,[55][56][57][58][59][60][61][62]. Under certain conditions, they may even be sensitive to the direction of the deposited momentum [63].…”
mentioning
confidence: 99%