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Non-dispersive wave packets in periodically driven quantum systems

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416 A. Buchleitner et al. / Physics Reports 368 (2002) 409–547<br />

one obta<strong>in</strong>s<br />

9W (˜r; ˜p; t)<br />

= {H; W (˜r; ˜p; t)} ; (22)<br />

9t<br />

where {:;:} denotes the classical Poisson bracket [3]: 3<br />

{f; g} = <br />

i=1:::f<br />

9f<br />

9ri<br />

9g<br />

9pi<br />

− 9f<br />

9pi<br />

9g<br />

9ri<br />

: (23)<br />

Eq. (22) is noth<strong>in</strong>g but the classical Liouville equation [3] which describes the classical evolution<br />

of a phase space density. Hence, <strong>in</strong> the “semiclassical limit” ˝ → 0, the Wigner density evolves<br />

classically. Corrections of higher power <strong>in</strong> ˝ can be calculated systematically. For example, the next<br />

order is ˝3H 3W=24 <strong>in</strong> Eq. (20), and generates terms which conta<strong>in</strong> third-order derivatives (<strong>in</strong> either<br />

position and=or momentum) of the Hamiltonian. Therefore, for a Hamiltonian of maximal degree<br />

two <strong>in</strong> position and=or momentum, all higher-order terms <strong>in</strong> Eq. (20) vanish and the Wigner distribution<br />

follows the classical evolution for an arbitrary <strong>in</strong>itial phase space density, and for arbitrarily<br />

long times. The harmonic oscillator is an example of such a system [2,16], <strong>in</strong> agreement with our<br />

discussion of Eq. (15) above.<br />

Now, once aga<strong>in</strong>, why does a <strong>wave</strong> packet spread? At rst sight, it could be thought that this<br />

is due to the higher-order terms <strong>in</strong> Eq. (20), and thus of <strong>quantum</strong> orig<strong>in</strong>. This is not true and<br />

spread<strong>in</strong>g of a <strong>wave</strong> packet has a purely classical orig<strong>in</strong>, as illustrated by the follow<strong>in</strong>g example.<br />

Let us consider a one-dimensional, free particle (i.e., no potential), <strong>in</strong>itially described by a Gaussian<br />

<strong>wave</strong> function with average position z0, average momentum p0 ¿ 0, and spatial width :<br />

<br />

1<br />

(z; t =0)= √ exp i<br />

1=4 p0z<br />

2 (z − z0)<br />

−<br />

˝ 2 2<br />

<br />

: (24)<br />

The correspond<strong>in</strong>g Wigner distribution is a Gaussian <strong>in</strong> phase space:<br />

W (z; p; t =0)= 1<br />

˝ exp<br />

<br />

2 2 (z − z0) (p − p0)<br />

− − 2<br />

2<br />

˝2 <br />

: (25)<br />

As the Hamiltonian is quadratic <strong>in</strong> the momentum, without potential, this distribution evolves precisely<br />

alike the equivalent classical phase space density. Hence, the part of the <strong>wave</strong> packet with<br />

p¿p0 will evolve with a larger velocity than the part with p¡p0. Even if both parts are <strong>in</strong>itially<br />

localized close to z0, the contribution of di erent velocity classes implies that their distance will<br />

<strong>in</strong>crease without bound at long times. The <strong>wave</strong> packet will therefore spread, because the various<br />

classical trajectories have di erent velocities. Spread<strong>in</strong>g is thus a completely classical phenomenon.<br />

This can be seen quantitatively by calculat<strong>in</strong>g the exact <strong>quantum</strong> evolution. One obta<strong>in</strong>s<br />

W (z; p; t)= 1<br />

˝ exp<br />

<br />

− (z − z0 − pt=m) 2<br />

2<br />

−<br />

2 (p − p0) 2 <br />

3<br />

We choose here the most common de nition of the Poisson bracket. Note, however, that some authors [14,15] use<br />

the opposite sign.<br />

˝ 2<br />

(26)

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