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Superconducting THz Transmission Spectrometer Comprising Josephson Oscillator and Cold-Electron Bolometer M.Tarasov, L.Kuzmin, E.Stepantsov, I.Agulo, A.Kalabukhov,

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Presentation on theme: "Superconducting THz Transmission Spectrometer Comprising Josephson Oscillator and Cold-Electron Bolometer M.Tarasov, L.Kuzmin, E.Stepantsov, I.Agulo, A.Kalabukhov,"— Presentation transcript:

1 Superconducting THz Transmission Spectrometer Comprising Josephson Oscillator and Cold-Electron Bolometer M.Tarasov, L.Kuzmin, E.Stepantsov, I.Agulo, A.Kalabukhov, T.Claeson Title

2 Outline Cold electron bolometer concept Bolometer samples Josephson oscillators Experimental setup Terahertz response Josephson and thermal radiation Conclusion

3 CEB chip layout 4 junction structure for cooling/heating Log-periodic antenna for 0.2-2 THz range Double-dipole antenna for 600 GHz Double-dipole antenna for 300 GHz

4 Center part of LPA Logperiodic antenna designed for frequency range 0.2- 2THz. Absorber length is 10  m

5 LPA SEM image Double dipole antenna designed for 300 GHz central frequency

6 SEM view of the LPA center SINIS bolometer inside the double dipole antenna. Absorbel length is 10  m

7 AFM picture of CEB

8 He3 sorption cooler

9 Quasioptical schematics JJ oscillator CEB

10 Sample holders Quasioptical sample holders with silicon and sapphire extended hyperhemisphere lenses and pogo- pins for contacts

11 Back-to-back configuration

12 Sample holder

13 YBaCuO film on tilted substrate SPM view of the 250 nm YBaCuO film on 14 o tilted sapphire substrate. Subgrains are elongated in the a-b plane perpendicular to tilt direction

14 Bicrystal Josephson junction SPM view of the YBaCuO bridge across the bicrystal grain boundary. Bridge length is 5  m, width below 1  m.

15 Josephson chip layout

16 IV curve and Shapiro steps IV curve of Josephson junction at 4.2 K without radiation (dashed) and under 300 GHz irradiation when critical current is completely suppressed

17 Current and voltage response Response of a 10 k  bolometer measured at 260 mK by applying a dc power to external junctions

18 Josephson radiation and overheating Radiation from a 55  Josephson junction with I c =10  A and when ctritical current is suppressed to zero by magnetic field

19 Overheating of the Josephson junction Temperature of the Josephson microbridge Planck’s radiation law, neglecting Tp For our design frequency 300 GHz and bias range up to 5 mV, it can be roughly fitted with the approximate expression

20 Log-periodic and double dipole Response of bolometer with a double-dipole antenna (black) and a log-periodic antenna (blue) under rediation from the same Josephson junction with log-periodic antenna

21 Magnetic field influence Signal from a Josephson junction with I c =400  A (black) and suppressed down to 150  A (blue), measured by bolometer with a double-dipole antenna

22 Terahertz response Dependence of bolometer response on the frequency of the first harmonic of Josephson oscillations. Last maximum corresponds to 1.7THz.

23 Conclusion We demonstrated the response of a normal metal cold electron bolometer at frequencies up to 1.7 THz. A voltage response of the bolometer is 4. 10 8 V/W and an amplifier-limited technical noise equivalent power 1.3. 10 -17 W/Hz 1/2. We were first to use electrically tunable high critical temperature Josephson quasioptical oscillator as a source of radiation in the range 0.2-2 THz. A high critical temperature Josephson junction operated at temperature about 2 K shows a I c R n product over 4.5 mV that enables an oscillation frequency over 2 THz. Combination of a Terahertz-band Josephson junction and a hot electron bolometer brings a possibility to develop a quasioptical cryogenic compact transmission spectrometer with a resolution of about 1 GHz. Such cryogenic spectrometer can be used for low-temperature spectral evaluation of any cryogenic detector, quasioptical submm wave grid filter, neutral density filter, absorber, etc. Cold electron bolometer detected that a Josephson junction is overheated by a transport current even when it is placed on millikelvin stage.

24 Per aspera ad astra


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