Squeezed light is a quantum state of light with reduced noise in one quadrature, used for precision measurements.Squeezed light is a quantum state of the electromagnetic field in which the uncertainty (noise) in one quadrature — one of the two complementary components of the field's oscillation, such as amplitude or phase — is reduced below the standard quantum limit, at the cost of increased noise in the other quadrature. This is possible because of Heisenberg's uncertainty principle, which allows redistributing quantum fluctuations between complementary variables as long as their product remains above the minimum. Squeezed light matters because it enables measurements with precision beyond what classical light allows, making it a cornerstone of quantum-enhanced metrology and a key resource for quantum information technologies.
The concept of squeezed light was first proposed by Carlton Caves in 1981, who showed that injecting squeezed vacuum into the unused port of an interferometer could reduce the quantum noise floor. The first experimental generation of squeezed light was achieved in 1985 by Richard Slusher and colleagues at Bell Labs.
In a coherent laser beam, the quantum noise is equally distributed between amplitude and phase quadratures, setting the standard quantum limit. Squeezing is achieved by passing light through a nonlinear optical medium, such as a specially designed crystal, where the interaction with the field creates correlations between photons. This process, called parametric down-conversion or four-wave mixing, effectively 'squeezes' the uncertainty ellipse of the field state: one quadrature becomes quieter (squeezed) while the orthogonal one becomes noisier (anti-squeezed). The squeezed quadrature can then be used as a low-noise probe for measuring tiny signals, such as phase shifts in interferometers, beating the classical shot-noise limit.
Squeezed light is used in gravitational wave detectors like LIGO and Virgo to enhance sensitivity, and in quantum key distribution and quantum imaging to improve signal-to-noise ratios beyond classical limits.
LIGO's gravitational wave detectors use squeezed light to reduce quantum noise, effectively making them sensitive enough to detect ripples in spacetime from collisions of black holes billions of light-years away.
| ⟨N⟩ | variable | mean particle number — particle number |
| r | variable | squeeze parameter — squeeze parameter |










