
Methods to minimize quantum noise in detectors, enhancing sensitivity for weak signal measurement.Quantum noise reduction is a collection of methods for suppressing the fundamental fluctuations that arise from the quantum nature of measurement. Even a perfect detector is limited by shot noise — the random arrival of photons or electrons — and by zero-point fluctuations of the measuring apparatus. Quantum noise reduction techniques, such as squeezing, back-action evasion, and quantum non-demolition measurements, allow researchers to push sensitivity beyond the standard quantum limit, making it possible to detect signals that would otherwise be buried in noise.
The concept of squeezing was introduced in the 1970s by Carlton Caves and others, with the first experimental demonstrations in the mid-1980s. The application to gravitational-wave detectors was proposed by Caves in 1981, and squeezed light has been used in LIGO since 2019.
The most common approach is squeezing: redistributing quantum noise so that one observable (say, the phase of a light beam) has less noise than the vacuum level, at the expense of the conjugate observable (amplitude). In interferometers, squeezed light injected into the dark port reduces the phase noise, improving sensitivity. For mechanical detectors, back-action evasion uses carefully timed measurements to avoid disturbing the motion being measured. Quantum non-demolition measurements repeatedly measure the same observable without perturbing it, allowing signal accumulation over time. These techniques often require cryogenic cooling and sophisticated feedback loops to isolate the system from classical noise sources.
Quantum noise reduction is essential in gravitational-wave observatories, atomic clocks, quantum sensors for dark matter searches, and any precision measurement where the standard quantum limit is the bottleneck.
The first gravitational-wave detection in 2015 was made without squeezing, but by 2019, LIGO's sensitivity had been improved by about 40% simply by injecting squeezed light — a purely quantum trick.
| LOD | variable | limit of detection — limit of detection mole per cubic metre |
| k | variable | confidence factor (typically 3) — confidence factor |
| σ_noise | variable | standard deviation of the blank signal — noise standard deviation |
| sensitivity | variable | slope of calibration curve (signal per concentration) — sensitivity cubic metre per mole |













