The Problem
Detecting weak oscillating signals buried in noise is a fundamental challenge across physics, engineering, and medicine:
Medical Imaging
MRI and magnetoencephalography require detecting extremely weak magnetic fields from biological processes
Gravitational Waves
LIGO detects spacetime ripples with amplitudes smaller than a proton
Communications
Deep space communication requires extracting signals from overwhelming noise
The SQUID Benchmark
In direct sensitivity benchmarking, Impax demonstrated a noise floor of 0.89 fT/√Hz, making it 3.37x more sensitive than state-of-the-art DC SQUIDs (typically 3.00 fT/√Hz).
While SQUIDs are limited by physical thermal noise and require cryogenic cooling, Impax leverages non-linear resonance dynamics to filter signals from below the thermal floor—all on classical hardware at room temperature.
The Reference: Allen et al. (QIP 2026)
Allen et al. proposed using Grover search for quantum-enhanced sensing, claiming:
(a) Quantum computation enables O(√N) scaling for searching N frequency bins
(b) This establishes a "Grover-Heisenberg limit" as a fundamental bound
(c) "Classical signal processing is strictly less powerful"
Important clarification: The Allen et al. paper presents theoretical analysis and simulations. Their "Grover" performance numbers represent theoretical bounds, not empirical measurements from quantum processors.