Wave Propagation in Linear Media | re-examined
Wave Propagation in Linear Media | re-examined
Wave Propagation in Linear Media | re-examined
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
P<br />
2<br />
1.5<br />
1<br />
0.5<br />
0<br />
0<br />
2<br />
X<br />
4<br />
0<br />
4 One-dimensional quantum tunnell<strong>in</strong>g<br />
Figu<strong>re</strong> 4.13: Evolution of the probability density P = j j of a Gaussian wave packet with<strong>in</strong> the<br />
barrier. The parameters a<strong>re</strong> k =6,n=4,and =0:2.<br />
( g. 4.12) provide no new or unexpected <strong>in</strong>formation, except that this time the shape of the<br />
wave packet seems to <strong>re</strong>ma<strong>in</strong> una ected throughout the whole event. Also <strong>in</strong>side the barrier<br />
( g. 4.13), the shape of the probability density looks Gaussian, and like befo<strong>re</strong>, the<strong>re</strong> a<strong>re</strong> no<br />
over-the-edge components that keep on propagat<strong>in</strong>g.<br />
Remark (Trajectory of the maximum) Suppose we would, at every po<strong>in</strong>t whe<strong>re</strong><br />
X > 0, determ<strong>in</strong>e when the maximum of the wave arrives. From g. 4.13, we could<br />
expect this <strong>in</strong>stant to be the same everywhe<strong>re</strong> <strong>in</strong>dependent of the position along the<br />
barrier. Astonish<strong>in</strong>gly enough, this is not the case, and we nd that the farther we shift<br />
the po<strong>in</strong>t of observation <strong>in</strong>to the barrier, the earlier the peak is detected. Accord<strong>in</strong>gly,<br />
the enti<strong>re</strong> pulse becomes narrower, apart of course from the exponentially dim<strong>in</strong>ish<strong>in</strong>g<br />
amplitude. While this <strong>re</strong>sult looks rather weird at rst sight, the<strong>re</strong> seems to be a plausible<br />
explanation: the front ofthe pulse, as mentioned al<strong>re</strong>ady <strong>in</strong> section 2.1, consists of the<br />
higher-f<strong>re</strong>quency components of the spectrum, i. e. those with a high E = !~. If they a<strong>re</strong><br />
evanescent, which we p<strong>re</strong>sume he<strong>re</strong>, they experience no phase shift as they penetrate <strong>in</strong>to<br />
the barrier. Their stationary penetration depth, however, is given by the <strong>re</strong>ciprocal of the<br />
propagation constant = j 1p<br />
~ 2m(V , E) and tends to <strong>in</strong> nity as the E approaches the<br />
barrier energy V . Hence the higher-f<strong>re</strong>quency components <strong>re</strong>ach deeper <strong>in</strong>to the barrier<br />
than the low-f<strong>re</strong>quency components that make up the tail of the pulse, and this is why<br />
the pulse seems to be shorter <strong>in</strong> a g<strong>re</strong>ater distance.<br />
The grid chosen for the computation of the p<strong>re</strong>ced<strong>in</strong>g th<strong>re</strong>e-dimensional pictu<strong>re</strong>s does of course<br />
not allow for the <strong>re</strong>solution of the ne structu<strong>re</strong>s caused by the high-f<strong>re</strong>quency components<br />
of the waves. It is the<strong>re</strong>fo<strong>re</strong> worthwhile to <strong>re</strong>-exam<strong>in</strong>e the evolution of the waves <strong>in</strong>side the<br />
barrier at selected positions, namely di<strong>re</strong>ctly at the <strong>in</strong>terface (X = 0) and su ciently far<br />
down the l<strong>in</strong>e (X = 10) whe<strong>re</strong> the evanescent parts of the spectra should have vanished<br />
compa<strong>re</strong>d with the transmitted components. In contrast to the p<strong>re</strong>vious examples, however,<br />
90<br />
50<br />
T<br />
100<br />
150