Characterization of escape times of Josephson Junctions for signal detection

TL;DR

This paper investigates how escape times of Josephson Junctions can be used for signal detection, identifying resonant behaviors and comparing detection strategies, with potential applications in weak signal analysis.

Contribution

It introduces an optimal likelihood ratio test for escape time detection, outperforming naive methods, and explores parameter estimation and practical applications.

Findings

Likelihood ratio test outperforms sample mean detector.

Resonant regions include stochastic and geometric resonance.

Performance approaches the Cramer-Rao bound in feasible detectors.

Abstract

The measurement of the escape time of a Josephson junction might be used to detect the presence of a sinusoidal signal embedded in noise when standard signal processing tools can be prohibitive. We show that the prescriptions for the experimental set-up and some physical behaviors depend on the detection strategy. More specifically, by exploiting the sample mean of escape times to perform detection, two resonant regions are identified. At low frequencies there is a stochastic resonance/activation phenomenon, while near the plasma frequency a geometric resonance appears. The naive sample mean detector is outperformed, in terms of error probability, by the optimal likelihood ratio test. The latter exhibits only geometric resonance, showing monotonically increasing performance as the bias current approaches the junction critical current. In this regime the escape times are vanishingly small and therefore performance are essentially limited by measurement electronics. The behavior of the likelihood ratio and sample mean detector for different values of incoming signal to noise ratio are discussed, and a relationship with the error probability is found. The likelihood ratio test based detectors could be employed also to estimate unknown parameters in the applied input signal. As a prototypical example we study the phase estimation problem of a sinusoidal current, that is accomplished by using the filter bank approach. Finally we show that for a physically feasible detector the performances are found to be very close to the Cramer- Rao theoretical bound. Applications might be found for example in some astronomical detection problems or to analyze weak signals in the sub-terahertz range.