Wave Propagation in Linear Media | re-examined
Wave Propagation in Linear Media | re-examined
Wave Propagation in Linear Media | re-examined
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4 One-dimensional quantum tunnell<strong>in</strong>g<br />
the tunnel and bounces back aga<strong>in</strong>, a fraction of it seems to get caught <strong>in</strong> the barrier, runn<strong>in</strong>g<br />
back and forth between the <strong>in</strong>terfaces while decay<strong>in</strong>g not too quickly. This peculiar e ect<br />
has noth<strong>in</strong>g to do with evanescent waves but stems from the ord<strong>in</strong>arily transmitted parts<br />
of the spectrum. It is just the common observation made for propagat<strong>in</strong>g waves that every<br />
change <strong>in</strong> the medium <strong>in</strong>evitably causes <strong>re</strong> ections. Look<strong>in</strong>g ca<strong>re</strong>fully, we even discover a<br />
small after-runner of the <strong>re</strong> ected wave (at T = 40 and X ,20 <strong>in</strong> the th<strong>re</strong>e-dimensional<br />
plot), which can be traced back to the <strong>in</strong>stant when the wave <strong>in</strong>side the barrier hits the left<br />
<strong>in</strong>terface (at X = 0) for the rst time.<br />
To <strong>in</strong>vestigate this behaviour <strong>in</strong> g<strong>re</strong>ater detail, we <strong>re</strong>gard an even thicker barrier and the same<br />
electron as befo<strong>re</strong> (as <strong>in</strong> the close-up of g. 4.22). In this case, the bounc<strong>in</strong>g of the wave <strong>in</strong>side<br />
the barrier is mo<strong>re</strong> marked, and each time it <strong>re</strong>aches an <strong>in</strong>terface, a small wave is <strong>re</strong>leased to<br />
the outside. This way, apart from the widen<strong>in</strong>g of the pulse due to dispersion, the <strong>in</strong>ner wave<br />
gradually fades away.<br />
Return<strong>in</strong>g to the orig<strong>in</strong>al example, we exam<strong>in</strong>e the trajectory of the peak of the wave packet<br />
( g. 4.23). To determ<strong>in</strong>e this path, we havetwo possibilities to identify the maximum (see also<br />
the discussion <strong>in</strong> section 1.5): a temporal and a spatial one. He<strong>re</strong> we consider the temporal<br />
maximum, i. e. the moment <strong>in</strong> time for a given position <strong>in</strong> space when the observed eld <strong>re</strong>aches<br />
its maximum amplitude. We <strong>re</strong>cognise the l<strong>in</strong>ear motion of the <strong>in</strong>cident and transmitted wave,<br />
as well as the not surpris<strong>in</strong>g fact that a de nition of the peak's trajectory is not mean<strong>in</strong>gful<br />
<strong>in</strong> the <strong>in</strong>terfe<strong>re</strong>nce zone <strong>in</strong> front of the barrier. Inte<strong>re</strong>st<strong>in</strong>gly enough, the trajectory of the<br />
transmitted wave is mo<strong>re</strong> strongly <strong>in</strong>cl<strong>in</strong>ed towards the axis than the <strong>in</strong>cident wave packet,<br />
mean<strong>in</strong>g that the packet to the right of the barrier runs faster. Aga<strong>in</strong>, this is largely due to<br />
the spectral components that can propagate over the barrier, whe<strong>re</strong>as the evanescent parts a<strong>re</strong><br />
enti<strong>re</strong>ly attenuated by the thick obstacle. Hence the low-f<strong>re</strong>quency components a<strong>re</strong> lte<strong>re</strong>d<br />
out, and the wave packet emanat<strong>in</strong>g from the far side of the barrier now has a spectrum that<br />
is narrower, but cent<strong>re</strong>d about a higher f<strong>re</strong>quency than befo<strong>re</strong>. He<strong>re</strong> and <strong>in</strong> the subsequent<br />
examples, the actual cent<strong>re</strong> f<strong>re</strong>quencies for both the <strong>in</strong>com<strong>in</strong>g and transmitted wave packets<br />
a<strong>re</strong> computed from the trajectories and given <strong>in</strong> the captions of the <strong>re</strong>spective gu<strong>re</strong>s. In the<br />
cur<strong>re</strong>nt example, this cent<strong>re</strong> f<strong>re</strong>quency is even above the cuto f<strong>re</strong>quency of the barrier. The<br />
propagation of the high-f<strong>re</strong>quency part is also <strong>re</strong>sponsible for the s-like shape of the trajectory<br />
with<strong>in</strong> the barrier and the o set between the extrapolated trajectories of the <strong>in</strong>cident and<br />
transmitted waves.<br />
It is not di cult to calculate the actual cent<strong>re</strong> f<strong>re</strong>quency from the trajectories. S<strong>in</strong>ce the<br />
wave packets a<strong>re</strong> smooth and well-behaved, we may safely take the view of the phase time<br />
supporters and assume that the wave proceeds at the group velocity, which wehavefound to<br />
be<br />
r<br />
2~!<br />
vg = :<br />
m<br />
(4.60)<br />
It is easy to t a straight l<strong>in</strong>e <strong>in</strong>to the space-time po<strong>in</strong>ts of the trajectory outside the barrier<br />
and away from the <strong>in</strong>terfe<strong>re</strong>nce <strong>re</strong>gion, and from the normalised variables, we obta<strong>in</strong> di<strong>re</strong>ctly<br />
102