2016
DOI: 10.1103/physrevb.93.024514
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Effects of nonequilibrium quasiparticles in a thin-film superconducting microwave resonator under optical illumination

Abstract: We have illuminated a thin-film superconducting Al lumped-element microwave resonator with 780 nm light and observed the resonator quality factor and resonance frequency as a function of illumination and microwave power in the 20 to 300 mK temperature range. The optically-induced microwave loss increases with increasing illumination but decreases with increasing microwave power. Although this behavior may suggest the presence of optically activated two-level systems, we find that the loss is better explained b… Show more

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Cited by 8 publications
(8 citation statements)
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References 47 publications
(62 reference statements)
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“…However, we note that gap broadening may also explain some of the structure in the residuals shown in Figure 3. The scale factors α x = 0.168 and α q = 0.106 are reasonable when interpreted as kinetic inductance fractions, and similar differences in the loss and fractional frequency responses have been observed in other aluminum resonators 23 . Non-dissipative quasiparticle states that affect x but not Q i have also been invoked to explain other MKID data 24 .…”
supporting
confidence: 77%
“…However, we note that gap broadening may also explain some of the structure in the residuals shown in Figure 3. The scale factors α x = 0.168 and α q = 0.106 are reasonable when interpreted as kinetic inductance fractions, and similar differences in the loss and fractional frequency responses have been observed in other aluminum resonators 23 . Non-dissipative quasiparticle states that affect x but not Q i have also been invoked to explain other MKID data 24 .…”
supporting
confidence: 77%
“…k B T ) (valid for T ≪ T c ) seems to match the measurement sufficiently well, where N 0 = 10 47 J −1 m −3 ≈ 1.74 × 10 4 μeV −1 μm −3 is the single spin electronic density of states at the Fermi level. [7,13] The fit to the frequency shift data is shown in Figure 3, and the extracted fitting parameters indicate that the aluminum superconducting gap at zero temperature is Δ S0 ≈ 170 μeV, a value close to the BCS gap approximation which is 1.76k B T c with transition temperature T c = 1.12 K. The values of the other fitting parameters are 𝛼 ≈ 0.014, and 𝛿 0 = 9.6 × 10 −6 . The values of 𝛼 and 𝛿 0 are consistent with other results on a variety of similar superconducting resonators.…”
Section: Frequency Shiftsmentioning
confidence: 80%
“…And eventually at high powers (𝜅 ≫ 1) such that w > 𝜈 for all temperatures, the equilibrium temperature dependence m = (1∕2) tanh (ℏ𝜔∕(2k B T)) in STM is recovered in the entire temperature range. The same discrete summation can be applied to Equation (13) for intermediate 𝛾 fluctuators. On the other hand, Equation (12) for high 𝛾 fluctuators is only modified with the substitution Γ 2 → √ Γ 2 2 + 𝜈 2 due to the sparse TLS assumption (See Section S3, Supporting Information).…”
Section: Fit To the Internal Loss Measurementsmentioning
confidence: 99%
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