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Wave Propagation in Linear Media | re-examined

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4.3 Examples of scatter<strong>in</strong>g processes<br />

P<br />

30<br />

2<br />

1.55<br />

1<br />

0.5 .5<br />

0<br />

0<br />

20<br />

10<br />

X<br />

10<br />

20<br />

T<br />

0<br />

30<br />

Figu<strong>re</strong> 4.8: Evolution of the probability density P = j j of a triangular wave packet with<strong>in</strong> the<br />

barrier. The parameters a<strong>re</strong> k =3and =0:8.<br />

40<br />

barrier energy T =1b= X=1b=<br />

0:3eV=4:8 10 ,20 J t =2:194 fs x =1:42 nm = 14:2A<br />

0:1eV=1:6 10 ,20 J t =6:582 fs x =2:46 nm = 24:6A<br />

Table 4.1: Actual dimensions for typical barriers.<br />

We now move on to triangular electrons, the spectrum of which is far mo<strong>re</strong> well-behaved<br />

than that of a <strong>re</strong>ctangular particle. For the rst example we use the same parameters as<br />

<strong>in</strong> the p<strong>re</strong>vious case. The behaviour outside the barrier ( g. 4.9) is essentially the same as<br />

befo<strong>re</strong>, but the wave forms a<strong>re</strong> much smoother now. The sharp peak of the <strong>in</strong>itial wave<br />

packet naturally disappears after a short time, and the <strong>re</strong> ected wave al<strong>re</strong>ady <strong>re</strong>sembles a<br />

Gaussian distribution. The same observation can be made for the part that penetrates the<br />

barrier ( g. 4.8). S<strong>in</strong>ce the parameters we<strong>re</strong> chosen such that a fairly large contribution still<br />

comes from the pass band, we <strong>re</strong>cognise a soft c<strong>re</strong>st mov<strong>in</strong>g ahead. Actually, the smoothlook<strong>in</strong>g<br />

wave function is superposed with small high-f<strong>re</strong>quent ripples that, like <strong>in</strong> the p<strong>re</strong>vious<br />

example, cannot be <strong>re</strong>solved <strong>in</strong> this plot.<br />

The wave packets conside<strong>re</strong>d so far we<strong>re</strong> ext<strong>re</strong>mely short (i. e. compris<strong>in</strong>g very few wavelengths<br />

of the carrier), which consequently <strong>re</strong>sulted <strong>in</strong> a broad spectrum. Let us now turn to the mo<strong>re</strong><br />

85

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