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Dark Count Reduction in Superconducting Nanowire Single Photon Detectors (SNSPDs)

ORAL

Abstract

Superconducting nanowire single photon detectors are the fastest single photon detectors with high detection efficiency, record time-resolution, and ultra-low dark count rate. However, for applications in dark matter search and quantum information, the dark count rate of SNSPDs must be further improved. In order to push these limits, we implemented a cryogenic differential bias-tee circuit, which filters high frequency noise from the current source and reduces electromagnetic noise coupling into the circuit thanks to a balanced architecture. We demonstrate that this differential architecture exhibits lower dark count rates compared to a single-ended device referenced to ground. We show, using a gaussian noise model, that the difference in dark counts for these two configurations can be attributed to electromagnetic noise.

Presenters

  • Hyunseong Kim

    Division of Physics, Mathematics and Astronomy, Caltech

Authors

  • Hyunseong Kim

    Division of Physics, Mathematics and Astronomy, Caltech

  • Andrew Mueller

    Division of Physics, Mathematics and Astronomy, Caltech

  • Boris Korzh

    Jet Propulsion Laboratory

  • Matthew Shaw

    Jet Propulsion Laboratory