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Non-dispersive wave packets in periodically driven quantum systems

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

SQUARED DIPOLE<br />

1.0<br />

0.5<br />

0.0<br />

ω−ω +<br />

ω<br />

ω+ ω−<br />

0.0 0.5 1.0 1.5 2.0<br />

Fig. 56. Square of the dipole matrix element (scaled w.r.t. n0, i.e., divided by n 2 0) connect<strong>in</strong>g the |0; 0; 0〉 non-<strong>dispersive</strong><br />

<strong>wave</strong> packet of a three-dimensional hydrogen atom <strong>in</strong> a circularly polarized micro<strong>wave</strong> eld with other Floquet states,<br />

as a function of the energy di erence between the two states. The stick spectrum is the exact result obta<strong>in</strong>ed from a<br />

numerical diagonalization with ! =1=60 3 , correspond<strong>in</strong>g to a pr<strong>in</strong>cipal <strong>quantum</strong> number n0 = 60, and scaled amplitude<br />

F0 =0:04446; <strong>in</strong> natural units, the micro<strong>wave</strong> frequency !=2 is 30:48 GHz, and the micro<strong>wave</strong> amplitude 17:6 V=cm.<br />

The crosses represent the analytic prediction with<strong>in</strong> the harmonic approximation [68]. There are three dom<strong>in</strong>ant l<strong>in</strong>es<br />

( + polarized) discussed <strong>in</strong> the text, other transitions (as well as transitions with − or polarizations) are negligible,<br />

what proves the validity of the harmonic approximation. If a weak probe eld (<strong>in</strong> the micro<strong>wave</strong> doma<strong>in</strong>) is applied to the<br />

system <strong>in</strong> addition to the driv<strong>in</strong>g eld, its absorption spectrum should therefore show the three dom<strong>in</strong>ant l<strong>in</strong>es, allow<strong>in</strong>g<br />

an unambiguous characterization of the non-<strong>dispersive</strong> <strong>wave</strong> packet.<br />

and the semiclassical energies observed <strong>in</strong> Figs. 30 and 59). This is not completely surpris<strong>in</strong>g as<br />

the energy levels themselves are well reproduced by this harmonic approximation, see Section 3.4.4.<br />

However, the photoabsorption spectrum probes the <strong>wave</strong> functions themselves (through the overlaps)<br />

which are well known to be much more sensitive than the energy levels. The good agreement for<br />

both the energy spectrum and the matrix elements is a clear-cut proof of the reliability of the<br />

harmonic approximation for physically accessible pr<strong>in</strong>cipal <strong>quantum</strong> numbers, say n0 ¡ 100; <strong>in</strong> fact,<br />

it is good down to n0 30, and the non-<strong>dispersive</strong> <strong>wave</strong> packet exists even for lower n0 values<br />

(e.g. n0 = 15 <strong>in</strong> [49]) although the harmonic approximation is not too good at such low <strong>quantum</strong><br />

numbers. There were repeated claims <strong>in</strong> the literature [30,44,46,54,62,144] that the stability island as<br />

well as the e ective potential are necessarily unharmonic <strong>in</strong> the vic<strong>in</strong>ity of the equilibrium po<strong>in</strong>t, and<br />

that the unharmonic terms will destroy the stability of the non-<strong>dispersive</strong> <strong>wave</strong> <strong>packets</strong>. The present<br />

results prove that these claims are doubly wrong: rstly, as expla<strong>in</strong>ed <strong>in</strong> Section 3.4.4, harmonicity<br />

is not a requirement for non-<strong>dispersive</strong> <strong>wave</strong>-<strong>packets</strong> to exist (the only condition is the existence of<br />

a su ciently large resonance island); secondly, the harmonic approximation is clearly a very good<br />

approximation even for moderate values of n0.<br />

Multiplication by the free space density of states transforms Fig. 56 <strong>in</strong> Fig. 57, which shows<br />

that the correspond<strong>in</strong>g spontaneous decay rates are very low, of the order of 100 Hz at most. They<br />

are few orders of magnitude smaller than the ionization rates and thus may be di cult to observe.<br />

With <strong>in</strong>creas<strong>in</strong>g n0, the spontaneous rate decreases algebraically while the ionization rate decreases<br />

exponentially, see Section 7.2.4. Thus for large n0, the spontaneous emission may be the dom<strong>in</strong>ant<br />

ωp

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