
A squeezed state is a quantum state with reduced noise in one variable at the expense of another, used in enhanced measurement and entanglement generation.A squeezed state is a nonclassical state of the electromagnetic field in which the variance (spread) of one quadrature variable (e.g., phase) becomes smaller than the vacuum level, while that of the conjugate becomes larger. Mathematically, it is obtained by applying the squeezing operator S(ζ) = exp[½(ζ* a² − ζ a†²)] to the vacuum or a coherent state. The parameter ζ = r e^{iθ} specifies the squeezing degree r and the direction in phase space. Such states are generated in nonlinear crystals via parametric down-conversion or four-wave mixing and are widely used to enhance the precision of interferometric measurements.
The first theoretical works belong to Yamamoto and Haus (1970s). In 1981, Carlton Caves showed the quantum-mechanical limits of interferometric measurements and proposed using squeezed light to overcome them. The experimental generation of squeezed states was first achieved by Slusher's group in 1985. In the 2000s, Rainer Weiss and colleagues developed a technique for injecting squeezed vacuum into gravitational detectors, which became one of the key achievements recognized by the 2017 Nobel Prize.
Squeezing is generated in a nonlinear crystal with χ⁽²⁾ susceptibility. In the parametric amplification regime, a pump photon with frequency ω_p decays into two entangled photons with frequencies ω_s and ω_i. If one of the beams is detected, conditional squeezing is realized in the other. In LIGO, squeezing of the vacuum state is used: squeezed vacuum is directed into the dark port of the Michelson interferometer, which reduces photocurrent fluctuations without introducing additional classical noise. The evolution equation in the Heisenberg picture for the quadratures is described by a linear squeezing transformation, preserving the commutation relations.
Allows gravitational-wave observatories to catch the shudder of space from black hole collisions, improving sensitivity by orders of magnitude.
In the LIGO detector, squeezed light reduces quantum noise so much that a length change of a four-kilometer arm by one-thousandth of a proton diameter can be noticed.
| ⟨N⟩ | variable | mean particle number — particle number |
| r | variable | squeeze parameter — squeeze parameter |
| z | variable | Squeezing parameter (complex) — squeezing parameter |
| â | variable | Annihilation operator — annihilation operator |
| ↠| variable | Creation operator — creation operator |
| exp[...] | operator | Exponentiation of an operator — exponential operator |
| c_s | variable | speed of sound — sound speed metre per second |
| P | variable | pressure — pressure pascal |
| \rho | variable | mass density — mass density kilogram per cubic metre |
| \left(\frac{\partial | operator | partial derivative with respect to density at constant entropy — partial derivative at constant entropy |
















