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Physical Review Letters

Creating Metastable Schrodinger Cat States

John J. Slosser, Gerard J Milburn

Published Sep 9, 1996• 2 citations
Publisher

Abstract

When the feedback process is optimized for minimum noise, the coefficient of the noise term [the second term in Eq. 9 of our paper] should be x not x 2 as stated.The value of x remains the same.The solutions go through much the same with this replacement throughout.This means that large values of x are not quite so serious as suggested by our original equation.In reality x is likely to be quite small, so a dependence on x rather than x 2 is unfortunate.I would like to thank Howard Wiseman for pointing out the incorrect dependence on x in our original paper.

DOI
10.1103/physrevlett.77.2344

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When the feedback process is optimized for minimum noise, the coefficient of the noise term [the second term in Eq. 9 of our paper] should be x not x 2 as stated.The value of x remains the same.The solutions go through much the same with this replacement throughout.This means that large values of x are not quite so serious as suggested by our original equation.In reality x is likely to be quite small, so a dependence on x rather than x 2 is unfortunate.I would like to thank Howard Wiseman for pointing out the incorrect dependence on x in our original paper.
Hydrodynamical equations for the probability density \ensuremath{\rho} and the local velocity v of a non-Markovian stochastic process have been recently obtained. The corresponding complex equation in terms of the wave function \ensuremath{\psi} coincides with the Schr\"odinger equation if the first-order terms only are retained. The second-order terms vanish and the third-order terms could be considered as QED-type corrections. To obtain the coefficient D4{\mathit{D}}_{4}D4​ of the third-order term the probability density \ensuremath{\rho} for a free particle is obtained by stochastic electrodynamics. This solution is substituted in the new complex equation, thus obtaining D4{\mathit{D}}_{4}D4​. By this coefficient the calculation of the Lyman-\ensuremath{\alpha} wavelength is in agreement with the best direct measurements for the transition 2P\ensuremath{\rightarrow}1S. The 1S displacement is 1% of the QED value for the Lamb shift. It is suggested how the new negative contribution could be the difference between the (1+0.01) QED value for the 3S state and the corresponding experimental value, which is 20% less than that given by QED.
We discuss the quantum-statistical properties of a system of absorbing atoms in a ring cavity under the action of a resonant classical field. At a semiclassical level, this system exhibits a bistable behavior in the sense that the transmitted light ET{E}_{T}ET​ is a discontinuous function of the incident light EI{E}_{I}EI​ with a hysteresis cycle, which resembles a first-order phase transition. Here we specify this analogy stressing the nonthermodynamic properties of this coherently driven system. The quantized field ET{E}_{T}ET​ is described by a Glauber PPP function, which obeys to a Fokker-Planck equation. This equation is derived from a very general master equation in the case of a good quality cavity by neglecting derivatives of order higher than second. A remarkable feature of this equation is that the diffusion coefficient is a nonlinear function of the field intensity. The steady-state solution of the Fokker-Planck equation has the following features. The PPP function can be single or double peaked according to the value of EI{E}_{I}EI​. In fact, our Fokker-Planck equation is like the one of a Brownian particle moving in a potential which presents one minimum or minima separated by a barrier, depending on the value of EI{E}_{I}EI​. The peaks of the PPP function correspond to the minima of the potential. In the double-peaked case, the peaks have different widths. The maxima of the ppp function occur at values of ET{E}_{T}ET​, which coincide with the classical stationary solutions that are stable according to the linear stability analysis. These semiclassical solutions give a discontinuous two-valued function of ET{E}_{T}ET​ vs EI{E}_{I}EI​ (hysteresis cycle). On the contrary, the mean value 〈ET〉〈{E}_{T}〉〈ET​〉 is a continuous single-valued function of EI{E}_{I}EI​, which behaves similarly to the Maxwell construction of a first-order phase transition: 〈ET〉〈{E}_{T}〉〈ET​〉 jumps from low to high values in a very sharp transition region of EI{E}_{I}EI​, which lies between the discontinuity points of the hysteresis cycle. However, the Maxwell rule that we obtain is quite different from that of equilibrium thermodynamics. The mean-square fluctuations of ET{E}_{T}ET​ are always very small except in the transition region where they are quite remarkable. We also present an exact expression of the stationary PPP function, which takes into account all higher-order derivatives, and we show that the Fokker-Planck approximation is very good for calculating mean values and mean-square fluctuations. Finally, we discuss the connections which link bistable absorption to the laser with injected signal and to the laser with a saturable absorber.
In this paper we establish three variational principles that provide new foundations for Nelson’s stochastic mechanics in the case of nonrelativistic particles without spin. The resulting variational picture is much richer and of a different nature with respect to the one previously considered in the literature. We first develop two stochastic variational principles whose Hamilton–Jacobi-like equations are precisely the two coupled partial differential equations that are obtained from the Schrödinger equation (Madelung equations). The two problems are zero-sum, noncooperative, stochastic differential games that are familiar in the control theory literature. They are solved here by means of a new, absolutely elementary method based on Lagrange functionals. For both games the saddle-point equilibrium solution is given by the Nelson’s process and the optimal controls for the two competing players are precisely Nelson’s current velocity v and osmotic velocity u, respectively. The first variational principle includes as special cases both the Guerra–Morato variational principle [Phys. Rev. D 27, 1774 (1983)] and Schrödinger original variational derivation of the time-independent equation. It also reduces to the classical least action principle when the intensity of the underlying noise tends to zero. It appears as a saddle-point action principle. In the second variational principle the action is simply the difference between the initial and final configurational entropy. It is therefore a saddle-point entropy production principle. From the variational principles it follows, in particular, that both v(x,t) and u(x,t) are gradients of appropriate principal functions. In the variational principles, the role of the background noise has the intuitive meaning of attempting to contrast the more classical mechanical features of the system by trying to maximize the action in the first principle and by trying to increase the entropy in the second. Combining the two variational principles, we get the quantum Hamilton principle, i.e., a variational characterization of the logarithm of the wave function ψ. The Lagrangian is the Lagrangian of classical mechanics with the complex-valued velocity v−iu replacing the classical velocity. The dynamics is given by a stochastic differential equation for real-valued diffusions with complex-valued drift and driving noise processes. From the variational principle we derive a Newton-type law. We finally define the momentum process and show that its mean and variance coincide with those of the quantum momentum operator.