A wideband, low-noise superconducting amplifier with high dynamic range
By Byeong Ho Eom, P. Day, H. Leduc, Jonas Zmuidzinas. Nature Physics, 2012
415 citations recorded by the source corpus.
An ideal amplifier has very low noise, operates over a broad frequency range, and has large dynamic range. Unfortunately, it is difficult to obtain all of these characteristics simultaneously. For example, modern transistor amplifiers offer multi-octave bandwidths and excellent dynamic range, but their noise remains far above the limit set by the uncertainty principle of quantum mechanics. Parametric amplifiers can reach the quantum-mechanical limit, but generally are narrow band and have very limited dynamic range. Here we describe a parametric amplifier that overcomes these limitations through the use of a travelling-wave geometry and the nonlinear kinetic inductance of a superconducting transmission line. We measure gain extending over 2 GHz on either side of an 11.56 GHz pump tone and place an upper limit on the added noise of 3.4 photons at 9.4 GHz. The dynamic range is very large, and the concept can be applied from gigahertz frequencies to ∼ 1 THz. An ideal amplifier has low noise, operates over a broad frequency range and has large dynamic range. A superconducting-resonator-based amplifier that combines all of these qualities is now demonstrated. The concept is applicable throughout the microwave, millimetre-wave and submillimetre-wave bands and can achieve a noise limit very close to that set by quantum mechanics.
Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Condensed Matter Physics
View Paper: https://www.semanticscholar.org/paper/7a392750abc9cc639cef1b40e1b7d024303eebff
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
Citations in the corpus
- ARCONS: A 2024 Pixel Optical through Near-IR Cryogenic Imaging Spectrophotometer (2013, background): “After this issue is addressed, lower noise microwave amplifiers (Ho Eom et al. 2012) and new MKID designs should continue to boost the resolution towards the theoretical limit.”
- The shape of the black hole photon ring: A precise test of strong-field general relativity (2020, background): “[29] B.”