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Non-dispersive wave packets in periodically driven quantum systems

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

a κ(q)<br />

250<br />

200<br />

150<br />

100<br />

50<br />

0<br />

−50<br />

−100<br />

−150<br />

−200<br />

−250<br />

0 50 100<br />

(a)<br />

q<br />

20<br />

10<br />

0<br />

−10<br />

−20<br />

0 1 2 3 4 5 6 7 8 9 10<br />

Fig. 9. Eigenvalues a (q) of the Mathieu equation, for a characteristic exponent = 0. These represent the energy levels<br />

of a pendulum as a function of the gravitational eld, see Eqs. (66) and (95). (a) Eigenvalues <strong>in</strong> the range [ − 2q; 2q]<br />

are associated with the librational bounded motion of the pendulum, while eigenvalues above 2q are associated with<br />

rotational modes. The dotted l<strong>in</strong>es represent the energies of the stable equilibrium po<strong>in</strong>t (lower l<strong>in</strong>e) and of the unstable<br />

equilibrium po<strong>in</strong>t (separatrix, upper l<strong>in</strong>e). Near the separatrix, the classical motion slows down and the quantal energy<br />

levels get closer. (b) Details for the rst excited states together with the semiclassical WKB prediction for the energy levels<br />

(- - -, Eqs. (39)). The semiclassical prediction is very accurate, except <strong>in</strong> the vic<strong>in</strong>ity of the separatrix.<br />

a (q) ≡ a ( =0;q) curves for the case of “optimal” resonance (see below), where n0 is an <strong>in</strong>teger<br />

and thus the characteristic exponent vanishes. Equivalently, the gure can be <strong>in</strong>terpreted as the<br />

evolution of the energy levels of a pendulum with the gravitational eld.<br />

The quasi-energy levels of the <strong>driven</strong> system can now be expressed as a function of a ( ; q):<br />

a κ(q)<br />

(b)<br />

<br />

E = H0(Î 1) − ! Î 1 − ˝<br />

<br />

+<br />

4<br />

˝2 ′′<br />

H 0 (Î 1) a ( ; q) : (102)<br />

8<br />

Together with Eqs. (98)–(100), this equation gives the quasi-energy levels of a <strong>periodically</strong> <strong>driven</strong><br />

system <strong>in</strong> the vic<strong>in</strong>ity of the resonance zone. The full, quasi-resonant part of the Floquet spectrum<br />

of the <strong>driven</strong> system is built from these quantized values through shifts k˝!, with arbitrary <strong>in</strong>teger<br />

values of k.<br />

A visual <strong>in</strong>spection of Fig. 9 immediately shows the existence of two regions <strong>in</strong> the energy<br />

diagram: with<strong>in</strong> the “<strong>in</strong>ner region”, |a ( ; q)| 6 2q, the energy levels form a regular fan of curves and<br />

tend to decrease with q. On the contrary, for a ( ; q) ¿ 2q, the energy levels <strong>in</strong>crease with q. Around<br />

a ( ; q)=2q, a transition region is visible with a series of apparent avoided cross<strong>in</strong>gs between the<br />

levels. This has a simple semiclassical explanation. The stable xed po<strong>in</strong>t of the pendulum described<br />

by the Mathieu equation (97) lies at v=0 with energy −2q, what expla<strong>in</strong>s why the a ( ; q) values are<br />

always larger. The unstable xed po<strong>in</strong>t has an energy +2q. Thus, <strong>in</strong> the range a ( ; q) ∈ [ − 2q; 2q],<br />

the pendulum is trapped <strong>in</strong> a region of librational motion. The energy levels can be approximated<br />

us<strong>in</strong>g the standard WKB quantization <strong>in</strong> the (Î; ˆ ) plane, as described <strong>in</strong> Section 3.1.1. The number<br />

q

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