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Non-dispersive wave packets in periodically driven quantum systems

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A. Buchleitner et al. / Physics Reports 368 (2002) 409–547 475<br />

with (see Eq. (166))<br />

V1(Î;M)=Î 2<br />

<br />

J ′ √ <br />

1 − e2 1(e) + sign(M) J1(e) ;<br />

e<br />

where (as <strong>in</strong> Eq. (124))<br />

<br />

(179)<br />

e =<br />

M 2<br />

1 −<br />

Î 2 : (180)<br />

However, the Maslov <strong>in</strong>dex for the (Î; ˆ ) motion is di erent. Indeed, the energy spectrum of the 2D<br />

atom is given by Eq. (116). Thus, quantized values of the action are half-<strong>in</strong>teger multiples of ˝. The<br />

relation between the resonant action Î 1 = ! −1=3 and the correspond<strong>in</strong>g pr<strong>in</strong>cipal <strong>quantum</strong> number<br />

now reads (with ˝ = 1):<br />

n0 = Î 1 − 1:<br />

(181)<br />

2<br />

As expla<strong>in</strong>ed <strong>in</strong> Section 3.1.4, the optimal case for the preparation of non-<strong>dispersive</strong> <strong>wave</strong> <strong>packets</strong>—<br />

where the states are the most deeply bound <strong>in</strong>side the resonance island—is for <strong>in</strong>teger values of n0,<br />

i.e., frequencies (cf. with Eqs. (65), (119))<br />

1<br />

! =<br />

: (182)<br />

(n0 +1=2) 3<br />

For the energy levels of the non-<strong>dispersive</strong> <strong>wave</strong> <strong>packets</strong>, this also implies that the characteristic<br />

exponents <strong>in</strong> the Mathieu equation—see Section 3.1.4—are shifted by one unit:<br />

= −2n0 (mod 2) = −2Î 1 + 1 (mod 2): (183)<br />

3.4.4. Transformation to the rotat<strong>in</strong>g frame<br />

The resonance analysis developed above is restricted to rst order <strong>in</strong> the amplitude F of the<br />

external drive. Extensions to higher orders are possible, but tedious. For CP, an alternative approach<br />

is possible, which allows higher orders to be <strong>in</strong>cluded quite easily. It is applicable to CP only and<br />

thus lacks the generality of the resonance approach we used so far. Still, it is rather simple and<br />

deserves an analysis.<br />

In CP, one may remove the time dependence of Hamiltonian (164) by a transformation to the<br />

non-<strong>in</strong>ertial frame rotat<strong>in</strong>g with the external frequency !. The unitary fransformation U =exp(i!Lzt)<br />

leads to [141,142]<br />

Hrot = UHCP U † 9U † ˜p2 1<br />

+iU = −<br />

9t 2 r + Fx − !Lz : (184)<br />

Classically, such an operation corresponds to a time-dependent rotation of the coord<strong>in</strong>ate frame<br />

spanned by x = x cos !t + y s<strong>in</strong> !t, y = y cos !t − x s<strong>in</strong> !t (and dropp<strong>in</strong>g the bar hereafter). 17<br />

17 Pass<strong>in</strong>g to the rotat<strong>in</strong>g frame implies a change of to = − !t <strong>in</strong> Eq. (165). That is de nitely di erent from the<br />

change → ˆ = − !t, Eq. (60), used <strong>in</strong> the resonance analysis. Both transformations are unfortunately known under the<br />

same name of “pass<strong>in</strong>g to the rotat<strong>in</strong>g frame”. This is quite confus<strong>in</strong>g, but one has to live with it. Along the resonantly<br />

<strong>driven</strong> circular orbit we are consider<strong>in</strong>g here, it happens that the azimuthal angle and the polar angle actually co<strong>in</strong>cide.<br />

It follows that the two approaches are equivalent <strong>in</strong> the vic<strong>in</strong>ity of this orbit.

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