Omega phase precipitation and superconducting critical transport currents in titanium-22 at. pct niobium /columbium/.
Omega phase precipitation and superconducting crital transport currents in Ti-Nb wire samples
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Omega phase precipitation and superconducting crital transport currents in Ti-Nb wire samples
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We describe superconducting diffusion-cooled hot-electron bolometers that were fabricated fromtantalum films grown on a thin niobium seed layer. The seed layer promotes single-phase growth of the Ta films, resulting in high-quality bolometers with transition temperatures up to 2.35 K and transition widths of less than 0.2 K. An S-parameter measurement set-up in a He-3 cryostat was used to measure device impedance versus frequency of a 400 nm long device at a temperature of 400 mK. It is shown that a 3 dB roll-off frequency of about 1 GHz can be achieved when the device resistance matches the impedance of the embedding network (no electrothermal feedback). This would lead to a prediction of 16 GHz for a 100 nm device, and indicates that a heterodyne mixer using a Ta HEB should be able to operate at several GHz even with a significant amount of electrothermal feedback.
We present a design for multipixel, multiband submillimeter instrument: SAMBA (Superconducting Antenna coupled, Multi-frequency, Bolometric Array).
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We describe a method for achieving arbitrary 1-qubit gates and controlled-NOT gates within the context of the Single Cooper Pair Box (SCB) approach to quantum computing. Such gates are sufficient to support universal quantum computation.
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We report on the first heterodyne measurements with a diffusion-cooled hot-electron bolometer.
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High frequency detector and circuit applications often require device fabrication on medium-to-low-dielectric constant substrates.
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