Bulletin of the American Physical Society
2024 APS March Meeting
Monday–Friday, March 4–8, 2024; Minneapolis & Virtual
Session Y52: Quantum Amplifiers II: Improvements and Applications
8:00 AM–11:00 AM,
Friday, March 8, 2024
Room: 201AB
Sponsoring
Unit:
DQI
Chair: Maxime Malnou, National Institute of Standards and Technology
Abstract: Y52.00006 : Characterization of Added Noise and Loss Mechanisms in Superconducting Kinetic Inductance Traveling Wave Parametric Amplifiers*
9:00 AM–9:12 AM
Presenter:
Logan Howe
(National Institute of Standards and Technology, Boulder; University of Colorado, Boulder)
Authors:
Logan Howe
(National Institute of Standards and Technology, Boulder; University of Colorado, Boulder)
Andrea Giachero
(University of Milano-Bicocca; INFN - Milano-Bicocca; National Institute of Standards and Technology, Boulder; University of Colorado, Boulder)
Michael R Vissers
(National Institute of Standards and Technology)
Jordan D Wheeler
(National Institute of Standards and Technology Boulder)
Jason Austermann
(National Institute of Standards and Technology, Boulder)
Johannes Hubmayr
(National Institute of Standards and Technology, Boulder)
Joel N Ullom
(National Institute of Standards and Technology)
Contemporary quantum technologies and fundamental physics experiments rely on amplifying and detecting extremely weak signals. As all amplifiers degrade the signal-to-noise-ratio by adding their own intrinsic noise, any amplifier which adds the minimum possible noise – referred to as the Standard Quantum Limit (SQL) – is of great value. In such settings parametric amplifiers are extremely attractive due to their ability to operate at, or very near, the SQL. Here we present a detailed characterization of the added noise of a superconducting Kinetic Inductance Traveling Wave Parametric Amplifier (KI-TWPA or KIT) capable of operating within two quanta of the SQL over 3 GHz of bandwidth. We perform an added noise characterization as a function of the operational KIT gain using the well-known y-factor technique, and independently using an intrinsically-calibrated shot noise Josephson tunnel junction. Additionally, using a vacuum noise squeezing setup, we explore the relationship between the squeezing level and added noise to further our understanding of sources of excess noise above the SQL in KITs.
*This work was supported in part by the National Aeronautics and Space Administration (NASA) Astrophysics Research and Analysis Program under grant numbers 80HQTR21T0023 and NNH18ZDA001N-APRA, by the Department of Energy (DOE) Accelerator and Detector Research Program under Grant No. 89243020SSC000058, and by DARTWARS, a project funded by the European Union’s H2020-MSCA under Grant No.101027746
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