10. Appendix
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Solution to Problem 2.16<br />
Solution to Problem 2.16 595<br />
(a) The matrix elements of the tight-binding Hamiltonian are given by (2.78).<br />
Examples of the calculation of these matrix elements, such as Hs2,s2, are given<br />
in the book for the diamond structure. The results for the zincblende structure<br />
differ only slightly from that of the diamond structure in that the two atoms<br />
in the unit cell are different. Since the nearest neighbor tetrahedral arrangement<br />
is the same in the two structures, one would expect that the definition<br />
of the vectors d1, ..., d4 would be the same. The main difference would be the<br />
matrix elements 〈S1|int|S1〉 and 〈S2|int|S2〉 which are no longer equal. Similarly<br />
〈X1|int|X1〉 would not be equal to 〈X2|int|X2〉 etc. This means that<br />
in Table 2.25 it would be necessary to introduce an energy ES1 for the matrix<br />
element 〈S1|int|S1〉 and a different energy ES2 for the matrix element<br />
〈S2|int|S2〉. Similarly, one can introduce energies Ep1 and Ep2.<br />
(b) At k 0, g0(k) 1 and g1(k) g2(k) g3(k) 0. Hence, the s-band<br />
determinant derived from the modified Table 2.25 for the zincblende crystal is<br />
given by:<br />
<br />
<br />
<br />
Es1 Es(0) Vss<br />
V∗ ss<br />
<br />
<br />
<br />
Es2 Es(0) 0<br />
Evaluating this determinant one obtains a quadratic equation in Es(0):<br />
[Es(0)] 2 Es(0)(Es1 Es2) (Es1Es2) |Vss| 2 0<br />
The solutions for the s-band energies at k 0 are therefore:<br />
Es(0) [(Es1 Es2)]/2] ± (1/2)[(Es1 Es2) 2 4|Vss| 2 ] 1/2<br />
The solutions for the p-band energies at k 0 can be obtained similarly.<br />
Solution to Problem 2.18<br />
In this case the overlap parameter Vxx can be evaluated in the same way as<br />
〈px|H|px〉 in Fig. 2.23 of the book and the result is the same, except for replacing<br />
the angle £ by £x.<br />
The overlap parameter Vxy can be evaluated, in principle, by drawing the<br />
following diagram and decomposing the figure into a sum of two figures as<br />
shown in Prob. 2.18-Fig. 1.<br />
The first figure on the right is rather simple and easy to calculate since<br />
both orbitals are projected along the vector d. The projections of px and py<br />
along d are simply px cos £x and py cos £y, respectively. The resulting overlap<br />
integral is VppÛ cos £x cos £y.<br />
The second overlap integral is more difficult to evaluate from the second<br />
figure on the right, since the components of px and py perpendicular to d are<br />
not parallel to each other. Instead, we will decompose the unit vector along