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Soviet physics. Doklady

Interference of zero-point fluctuations of the electromagnetic vacuum and photon corelation in parametric light scattering

G. Kh. Kitaeva, Alexander N. Penin, Alexander V. Sergienko

Published Apr 1, 1987• 0 citations
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The Scharnhorst effect in quantum electrodynamics predicts a superluminal velocity shift $δc>0$ at low photon frequencies due to vacuum fluctuations between two mirrors. Although theoretically robust (no causality violation), the effect is extraordinarily small ($δc/c\approx 10^{-32}$ for mirrors $1\,μ{\rm m}$ apart) and outside current experimental reach. Here we propose a condensed matter analogue, replacing the photons in the electromagnetic vacuum by phonon excitations of a Bose-Einstein condensate. In an idealized geometry, the two-dimensional surface of a cylinder (circumference $L$) at zero temperature, the axial speed of sound is increased due to zero-point fluctuations of the condensate by $δc/c\simeq 5\times 10^{-3}\,\tilde{g}$ at $L\simeq 2\,ξ$, to first order in the dimensionless interaction constant $\tilde{g}\simeq 10^{-1}$ of the Bose gas of healing length $ξ\simeq 1\,μ{\rm m}$. This is 28 orders of magnitude larger than the photonic effect, basically because phonons have a self-interaction while photons only interact via massive electrons. We discuss the prospects for observation of the acoustic Scharnhorst effect, the main restriction being the low-temperature requirement.

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Detection of amplitude modulation with squeezed light for sensitivity beyond the shot-noise limit

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An improvement in precision beyond the limit set by the vacuum-state or zero-point fluctuations of the electromagnetic field is reported for the detection of amplitude modulation encoded on a weak signal beam. The improvement is achieved by employing the squeezed light from an optical parametric oscillator to reduce the level of fluctuations below the shot-noise limit. An increase in signal-to-noise ratio of 2.5 dB relative to the shot-noise limit is demonstrated.

Optics Letters•Jun 1, 1988•63 citations
Frequency-angular distributions of signal wave intensity are calculated for spontaneous parametric down-conversion and parametric frequency conversion in spatially nonuniform nonlinear media. Wave reflection from interfaces is taken into account, and both regular and irregular nonuniform distributions of second-order nonlinear susceptibility are considered. A unified approach using a scattering matrix and a generalized Kirchhoff law is applied in calculations of spontaneous and stimulated processes in dissipative nonlinear media. Interference of electromagnetic zero-point fluctuations of the vacuum, nonlinear interference, and nonlinear diffraction are examined for media with various absorptive properties. Theoretical foundations are developed for diagnostics of nonuniform distributions of the second-order susceptibility, based on measurement of the line profiles of nonlinear signals.
The Scharnhorst effect in quantum electrodynamics predicts a superluminal velocity shift δc>0δc>0δc>0 at low photon frequencies due to vacuum fluctuations between two mirrors. Although theoretically robust (no causality violation), the effect is extraordinarily small (δc/c≈10−32δc/c\approx 10^{-32}δc/c≈10−32 for mirrors 1 μm1\,μ{\rm m}1μm apart) and outside current experimental reach. Here we propose a condensed matter analogue, replacing the photons in the electromagnetic vacuum by phonon excitations of a Bose-Einstein condensate. In an idealized geometry, the two-dimensional surface of a cylinder (circumference LLL) at zero temperature, the axial speed of sound is increased due to zero-point fluctuations of the condensate by δc/c≃5×10−3 g~δc/c\simeq 5\times 10^{-3}\,\tilde{g}δc/c≃5×10−3g~​ at L≃2 ξL\simeq 2\,ξL≃2ξ, to first order in the dimensionless interaction constant g~≃10−1\tilde{g}\simeq 10^{-1}g~​≃10−1 of the Bose gas of healing length ξ≃1 μmξ\simeq 1\,μ{\rm m}ξ≃1μm. This is 28 orders of magnitude larger than the photonic effect, basically because phonons have a self-interaction while photons only interact via massive electrons. We discuss the prospects for observation of the acoustic Scharnhorst effect, the main restriction being the low-temperature requirement.