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Physical Review A

Quantum collapses and revivals in an optical cavity

Tran Quang, P. L. Knight, V. Buek

Published Nov 1, 1991• 101 citations
Publisher

Abstract

We study the influence of the atomic spontaneous-emission decay on the collapse-revival phenomena in the optical region. We demonstrate that revivals of the atomic inversion are much more sensitive to cavity-field damping than to spontaneous emission. This suggests that the additional dissipation caused by spontaneous emission would not offer an insurmountable obstacle to the experimental observation of optical revivals in high-Q cavities.

DOI
10.1103/physreva.44.6092

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We study the influence of the atomic spontaneous-emission decay on the collapse-revival phenomena in the optical region. We demonstrate that revivals of the atomic inversion are much more sensitive to cavity-field damping than to spontaneous emission. This suggests that the additional dissipation caused by spontaneous emission would not offer an insurmountable obstacle to the experimental observation of optical revivals in high-Q cavities.
We present two simple soluble quantum optical models in which an atomic system is coupled to a bath containing an infinite number of reservoir states. The total system is treated conservatively, but the atomic subsystem of interest exhibits decay. The first system consists of a single two-level atom coupled to an infinite number of modes of a one-dimensional cavity which are equally spaced in frequency. The coupling results in spontaneous emission by an excited atom into the modes of the cavity. The model also exhibits the subsequent re-excitation of the atom after the spontaneously emitted radiation is reflected from the ends of the cavity. The second is a single two-level atom coupled to a single mode of a damped optical cavity where the damping is provided by coupling to quantized oscillators in the walls of the cavity. The damped cavity alters the spontaneous emission rate from its free space value. The simplicity of both models makes them attractive as a method for introducing quantum mechanical damping phenomena.
A single atom coupled to a quantized mode of an electromagnetic cavity, driven by an external coherent field, is described by the Hamiltonian H djc = ig(a†σ− − aσ+) + iε(a† − a), where (a†, a) and (σ+, σ) are the raising and lowering operators for the cavity mode and atom, respectively. This is the single atom version of the Hamiltonian used in the study of optical bistability. It describes the evolution of the atom-cavity system on time scales much smaller than the inverse spontaneous emission and cavity decay rates. For 2ε/g < 1, HDJC possesses a discrete set of interaction eigenstates1 with eigenvalues E n ± = ± g n [ 1 − ( 2 ε / g ) 2 ] 3 / 4 . These form a renormalized version of the usual Jaynes-Cummings eigenstates2, which correctly take into account the effect of the driving field to all orders of magnitude. We investigate the collapse and revival nature of the dynamical evolution of the single atom in a cavity, with and without dissipation and above and below the threshold 2ε/g = 1 of the driven Jaynes-Cummings Hamiltonian.
The collapse and revival of quantum states appear in diverse areas of physics. In quantum optics the occurrence of such a phenomena in the evolution of an atomic state, interacting with a light field initially in a coherent state, was predicted by using the Jaynes-Cummings model (JCM), and subsequently demonstrated experimentally. In this paper we revisit the JCM with the Monte-Carlo wave function approach and investigate the time evolution of the photon emission rate of the atom in a cavity. Analytical and numerical quantum trajectory calculations show that the cavity and the initial field statistics strongly influence the photon emission dynamics. A coherent field indeed gives rise to a collapse and revival behavior that mirrors atomic state evolution. However, there are differences between the two. The emission rate for a field in a Fock number state exhibits a sinusoidal oscillation, and there exists a quiescent period for a thermal field. These properties are quite different from those in free space. It is also shown that the fluctuation in photon emission is much less than that of the atomic population.