A degenerate optical parametric oscillator pumps a χ⁽²⁾ nonlinear crystal inside a resonant cavity with light at frequency 2ω. Pump photons split into pairs of identical "signal" photons at ω via spontaneous parametric down-conversion. Below the oscillation threshold the cavity builds up a vacuum field whose two quadratures — amplitude X₁ and phase X₂ — are squeezed asymmetrically instead of amplified together:
x = P_pump / P_threshold (0 ≤ x < 1)
x_eff = x / √(1 + (Δ/κ)²) (detuning weakens the parametric gain)
V₋(x_eff) = (1 − x_eff)/(1 + x_eff) squeezed quadrature variance
V₊(x_eff) = (1 + x_eff)/(1 − x_eff) anti-squeezed quadrature variance
n̄ = x_eff² / (1 − x_eff²) intracavity mean photon number
Shot-noise unit: V = 1. dB = 10·log₁₀(V)
- Pump power — sets x. As x → 1 the squeezed quadrature's noise is crushed toward zero while the conjugate quadrature's noise diverges — the Heisenberg product V₋·V₊ = 1 stays fixed even as the ellipse stretches.
- Cavity detuning — moving the cavity off two-photon resonance reduces the effective parametric interaction, so both squeezing and photon buildup weaken symmetrically for +Δ and −Δ.
- Cavity linewidth κ — sets how fast intracavity fluctuations decorrelate; only changes the animation timescale here, not the steady-state variances.
- LO / squeezing angle θ — a homodyne local-oscillator phase; rotates which quadrature you are looking at. The point cloud is the field's noise distribution in phase space — an ellipse, not a circle, is the signature of squeezing.
Real-world relevance: sub-threshold degenerate OPOs are the standard laboratory source of continuous-variable squeezed light, used in gravitational-wave detectors (LIGO's frequency-dependent squeezing) and continuous-variable quantum key distribution to beat the standard quantum limit.