2019
DOI: 10.1364/ol.44.001198
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Direct detection of the idler THz radiation generated by spontaneous parametric down-conversion

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Cited by 18 publications
(10 citation statements)
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“…Table 2 summarizes the main parameters of the studied VN structures with a sensitive area of 0.4 μm × 0.4 μm, as well as the experimentally obtained value of the ultimate noise equivalent power which amounted to NEP @1MHz = 6.3 × 10 –14 W/√Hz and the minimum energy level is equal δE ≈ 8.1 × 10 –18 J. For comparison, the same table presents the main parameters of the most common NbN HEB detectors, where NEP value is NEP = 2.5 × 10 –13 W/√Hz 5 , which is 4 times higher than NEP of the VN HEB detectors. Note that the indicated value of NEP of the VN HEB detectors can be further reduced by creating detectors with a smaller sensitive area.…”
Section: Experimental Nep Of the Vn Detectormentioning
confidence: 95%
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“…Table 2 summarizes the main parameters of the studied VN structures with a sensitive area of 0.4 μm × 0.4 μm, as well as the experimentally obtained value of the ultimate noise equivalent power which amounted to NEP @1MHz = 6.3 × 10 –14 W/√Hz and the minimum energy level is equal δE ≈ 8.1 × 10 –18 J. For comparison, the same table presents the main parameters of the most common NbN HEB detectors, where NEP value is NEP = 2.5 × 10 –13 W/√Hz 5 , which is 4 times higher than NEP of the VN HEB detectors. Note that the indicated value of NEP of the VN HEB detectors can be further reduced by creating detectors with a smaller sensitive area.…”
Section: Experimental Nep Of the Vn Detectormentioning
confidence: 95%
“…For example, the detection and study of the effect of electronic heating in superconducting NbN films, arising under the influence of radiation of different frequencies from the visible to the millimeter wave range, has led to the creation of a new class of cryogenic electronic devices 1 , 2 . One of these devices, of course, become superconducting NbN HEB (Hot-Electron Bolometer) detectors that exhibit high sensitivity (NEP ≈ 2 × 10 –13 W/√Hz) combined with record response time (τ ≈ 50 ps), as well as energy resolution δE ≈ 3 × 10 –18 J 3 5 . Such unique characteristics of NbN HEB detectors made possible by the use of ultra-thin (d ≈ 3–5 nm) disordered NbN films, which are characterized by a low diffusion coefficient (D ≈ 0.5 cм 2 /c), high critical temperature (T c ≈ 10 К), small width of the superconducting transition (∆T c < 0.2 К), the strong temperature dependence of the resistance in the region of the superconducting transition.…”
Section: Introductionmentioning
confidence: 99%
“…Thus, we can generalize Equation ( 7) for any type of discrete distribution () PN by taking Equation ( 8) instead of Equation (5). The relationship between statistical distribu-Figure 3.…”
Section: Figurementioning
confidence: 99%
“…Thus, we can generalize Equation ( 7) for any type of discrete distribution P(N) by taking Equation ( 8) instead of Equation (5). The relationship between statistical distributions of the bolometer readings P(z) and of the number of input photons P(N) takes the form…”
Section: Figurementioning
confidence: 99%
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