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Chinese Journal of Physics

Atomic Evolution in a Driven Gravitational Cavity

Farhan Saif

Published Aug 1, 2001• 0 citations
OpenAlex

Abstract

We propagate an atomic wavepacket in a gravitational cavity which is modulated by means of an external periodic driving force. We show that in classical evolution it displays classical chaos, whereas in the quantum domain the wavepacket exhibits dynamical localization. Moreover, we also find dynamical revivals in the quantum evolution and prove that this is a generic characteristics of all driven systems.

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We propagate an atomic wavepacket in a gravitational cavity which is modulated by means of an external periodic driving force. We show that in classical evolution it displays classical chaos, whereas in the quantum domain the wavepacket exhibits dynamical localization. Moreover, we also find dynamical revivals in the quantum evolution and prove that this is a generic characteristics of all driven systems.
Quantum revivals are investigated for the dynamics of an atom in a driven gravitational cavity. It is demonstrated that the external driving field influences the revival time significantly. Analytical expressions are presented which are based on second-order perturbation theory and semiclassical secular theory. These analytical results explain the dependence of the revival time on the characteristic parameters of the problem quantitatively in a simple way. They are in excellent agreement with numerical results.
We calculate the quantum revival time for a wave packet initially well localized in a one-dimensional potential in the presence of an external periodic modulating field. The dependence of the revival time on various parameters of the driven system is shown analytically. As an example of an application of our approach, we compare the analytically obtained values of the revival time for various modulation strengths with the numerically computed ones in the case of a driven gravitational cavity. We show that they are in very good agreement.
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.