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For the basic solution and the dispersion relation
(energy vs. momentum / wave vector) nothing has changed, and we obtain
(independent of boundary conditions) |
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| y |
= |
æ
ç
è |
1
L |
ö
÷
ø |
3/2 |
· |
exp (i · k · r) |
| E = |
2
· k2
2 m |
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Only the allowed values of the wave vector
k are determined by the boundary conditions; for the fixed
conditions given here we have |
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| y (x = 0) |
= |
y (x = L) = 0 |
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 |
Obviously this condition can be satisfied by
|
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|
| k |
= |
n · p
l |
| |
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| n |
= |
1, 2, 3, ... |
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|
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The number of states
Z(k) up to a wave vector k is
generally given by |
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| Z(k) |
= |
Volume of sphere with radius E(k)
Volume of state |
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 |
For fixed boundary conditions we
have |
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| Z(k) |
= |
1
8 |
· |
4/3 (p · k)3
(p/L)3 |
= |
(k · L)3
6p2 |
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This is exactly what we would get for
the periodic boundary conditions - thanks to the factor 1/8. |
|
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Where does this factor come from? Easy - since
the quantum numbers n are restricted to positive integers in this case,
we can not count states in 7 of the 8 octants of the complete
sphere and must divide the volume of the complete sphere by 8. |
|
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This becomes clear if we look at a drawing of the
possible states in phase space: |
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© H. Föll (Semiconductor - Script)