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Non-dispersive wave packets in periodically driven quantum systems

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

with Eqs. (40) and (65),<br />

<br />

dEn <br />

<br />

dn = ˝! : (87)<br />

n=n0<br />

Note that, by this de nition, n0 is not necessarily an <strong>in</strong>teger. In the semiclassical limit, where n0<br />

is large, the WKB approximation connects n0 to the center of the classical resonance island, see<br />

Eq. (39),<br />

n0 + 4 = Î 1<br />

˝<br />

; (88)<br />

En0 = H0(Î 1) ; (89)<br />

with be<strong>in</strong>g the Maslov <strong>in</strong>dex along the resonant trajectory. Furthermore, for n close to n0, we can<br />

expand the unperturbed energy at second order <strong>in</strong> (n − n0),<br />

En En0 +(n− n0)˝! + 1 d<br />

2<br />

2En dn2 <br />

<br />

(n − n0) 2 ; (90)<br />

n0<br />

where the second derivative d2En=dn 2 is directly related to the classical quantity H ′′<br />

0 , see Eq. (67),<br />

with<strong>in</strong> the semiclassical WKB approximation, Eq. (39). Similarly, the matrix elements of V are<br />

related to the classical Fourier components of the potential [7], Eq. (55),<br />

〈 n|V | n+1〉 〈 n+1|V | n+2〉 V1(Î 1) ; (91)<br />

evaluated at the center Î = Î 1—see Eq. (65)—of the resonance zone.<br />

With these <strong>in</strong>gredients and r = n − n0, Eq. (85) is transformed <strong>in</strong> the follow<strong>in</strong>g set of approximate<br />

equations:<br />

<br />

<br />

E − H0(Î 1)+! Î 1 − ˝<br />

<br />

−<br />

4<br />

˝2 ′′<br />

H 0 (Î 1)r<br />

2 2<br />

<br />

dr = V1(dr+1 + dr−1) ; (92)<br />

where<br />

dr ≡ cn0+r;n0+r : (93)<br />

Note that, because of Eq. (87), the r values are not necessarily <strong>in</strong>tegers, but all have the same<br />

fractional part.<br />

The tridiagonal set of coupled equations (92) can be rewritten as a di erential equation. Indeed,<br />

if one <strong>in</strong>troduces the follow<strong>in</strong>g function associated with the Fourier components dr:<br />

f( )= <br />

exp(ir )dr ; (94)<br />

Eq. (92) can be written as<br />

<br />

− ˝2<br />

2<br />

r<br />

H ′′<br />

0 (Î 1) d2<br />

d 2 + H0(Î 1) − !<br />

<br />

Î 1 − ˝<br />

<br />

+ V1 cos<br />

4<br />

<br />

f( )=Ef( ) ; (95)<br />

which is noth<strong>in</strong>g but the <strong>quantum</strong> version of the pendulum Hamiltonian, Eq. (66). Thus, the present<br />

calculation is just the purely <strong>quantum</strong> description of the non-l<strong>in</strong>ear resonance phenomenon. The

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