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10. Appendix

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plus<br />

Jz ·Fz<br />

Solution to Problem 5.7 631<br />

(5.6k)<br />

If there are both electrons and holes we have to add their contributions to J.<br />

Notice that · depends on the charge as q2 so ·n and ·p will both be positive.<br />

Similarly (5.6i) to (5.6k) are valid for both electrons and holes. Finally, if we<br />

assume that Bz is small then the B2 z terms can be neglected and the answer<br />

for J is:<br />

and<br />

Jx (·n ·p)Fx (‚n ‚p)FyBz<br />

Jy (·n ·p)Fy (‚n ‚p)FxBz<br />

Jz (·n ·p)Fz<br />

(b) In the Hall configuration Jy 0 in (5.6j) so that<br />

Fy Fx[(‚n ‚p)Bz/(·n ·p)] and<br />

Jx Fx[(·n ·p) 2 (‚n ‚p) 2 B 2 z ]/(·n ·p)<br />

The Hall Coefficient is RH Fy/JxBz (‚n ‚p)/[(·n ·p) 2 (‚n ‚p) 2B2 z ].<br />

Again, at low magnetic field, we can neglect the B2 z term so that<br />

RH (‚n ‚p)/(·n ·p) 2 .<br />

In terms of Nn and Np etc., the Hall Coefficient is equal to:<br />

RH (1/qc)[Np (Ìn/Ìp) 2 Nn]/[(Ìn/Ìp)Nn Np] 2<br />

Solution to Problem 5.7<br />

For samples where the electron distribution is given by f (E) the ensemble<br />

average of the current density is given by (5.88a) to(5.88c):<br />

and<br />

〈jx〉 ·Fx ÁBzFy<br />

〈jy〉 ·Fy ÁBzFx<br />

〈jz〉 〈Û0〉Fx<br />

where F and B are the electric and magnetic fields, respectively; · and Á are<br />

defined in (5.89a) and (5.89b). To obtain the Hall Coefficient RH we set 〈jy〉 <br />

0 so that Fy (Á/·)BzFx. Substituting back into RH Fy/〈Jx〉Bz we obtain:<br />

RH (Á/· 2 )Fx/[·Fx ÁBzFy] (Á/· 2 )/[1 (ÁBz/·) 2 ].

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