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Bulletin of the American Physical Society

Characterization of Low Noise Superconducting Microwave Amplifiers

Ted White, R. Barends, Joerg Bochmann, B. Chiaro, Y. Chen, Jack B. Kelly, M. Lenander, Erik A. Lucero, M. Mariantoni, A. Megrant, Charles Neill, P. J. J. O’Malley, P. Roushan, D. Sank, A. Vainsencher, J. Wenner, Yang Yin, Andrew N. Cleland, John M. Martinis

Published Feb 29, 2012• 0 citations
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We show an experimental study of superconducting X-mon qubit based on low noise wideband measurement setup. The setup includes wide stop-band low frequency filters with a stopband frequency up to 13 GHz, the broadband low-noise cryogenic microwave amplifier (cLNA) operating at 3.8 K. The obtained power dissipation of the cLNA is below 20 mW, the frequency operating ranges from 6 GHz to 12 GHz with a gain of 30 dB. The equivalent noise temperature of the amplifier is bellow 6 K for the presented frequency range. We demonstrate here the characterization of the superconducting X-mon qubit coupled to an on-chip coplanar waveguide resonator. We show standard qubit experiments: one and two-tones qubit spectroscopy, ac-Stark shift experiments for probing and excitation power sweeps.