1999
DOI: 10.1063/1.123388
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Intrinsic picosecond response times of Y–Ba–Cu–O superconducting photodetectors

Abstract: We report our femtosecond time-resolved measurements on the photoresponse of an epitaxial YBa 2 Cu 3 O 7Ϫx ͑YBCO͒ thin-film photodetector, patterned into a microbridge geometry. By varying the current-voltage biasing conditions between the superconducting and resistive ͑hot spot͒ states, we observed transients that correspond to the nonequilibrium kinetic-inductance and the nonequilibrium electron-heating response mechanisms, respectively. The two-temperature model and the Rothwarf-Taylor theory have been used… Show more

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Cited by 100 publications
(65 citation statements)
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References 17 publications
(18 reference statements)
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“…Typical intrinsic NbN detector response times are  ≈ 30 ps [28], [29]. For YBCO response times as short as single picoseconds were achieved [30], [31]. These detectors are much faster than commercial Ge or InSb bolometers that exhibit time constants in the microsecond or even millisecond range [32].…”
Section: Methodsmentioning
confidence: 99%
“…Typical intrinsic NbN detector response times are  ≈ 30 ps [28], [29]. For YBCO response times as short as single picoseconds were achieved [30], [31]. These detectors are much faster than commercial Ge or InSb bolometers that exhibit time constants in the microsecond or even millisecond range [32].…”
Section: Methodsmentioning
confidence: 99%
“…These receivers are noticeably noisier, compared to low temperature devices, as phonon dynamics play an appreciable role due to the relatively high operating tempe− rature and introduce of excess noise [225,226]. Actually, HTSC HEB mixers are not reaching the sensitivity of low temperature superconducting HEBs, but because of very short electron−phonon relaxation time (t eph »1.1 ps in YBaCuO [227] …”
Section: Superconducting Hot-electron Bolometersmentioning
confidence: 99%
“…The very short inelastic electron-phonon scattering time e-ph Ϸ2 ps at temperatures of about T Ϸ85-90 K allows one to suggest YBCO thin films for the development of hot-electron bolometer ͑HEB͒ mixers of electromagnetic radiation with a characteristic Ϫ3 dB rolloff frequency f ro up to 100 GHz. [2][3][4][5] This wide intermediate frequency ͑IF͒ bandwidth of the mixer is very important especially in the terahertz frequency range because of the lack of a tunable local oscillator ͑LO͒ for these frequencies. However, as shown in Ref.…”
Section: Introductionmentioning
confidence: 99%