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10. Appendix

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Solution to Problem 3.17 617<br />

forces holding the atoms together, and a second one stems from the vibration<br />

of the atoms. Since phonons are bosons (like photons), the calculation of<br />

the free energy term due to phonons is the same as that for photons and can<br />

be found in many standard textbooks on statistical mechanics (see, for example,<br />

C. Kittel and H. Kroemer: Thermal Physics, second edition. Freeman, San<br />

Francisco, 1980. p. 112). The contribution Fvib to the total free energy from<br />

the phonons can be calculated from the partition function Zvib of phonons:<br />

Fvib kBT ln Zvib where kB is the Boltzmann’s constant and<br />

Zvib <br />

1 (n<br />

e 2)<br />

i,n<br />

ˆi <br />

kBT e<br />

i<br />

ˆi 1<br />

2kBT 1 e ˆ <br />

i<br />

kBT 1<br />

(3.17.3)<br />

ˆi<br />

i 2 sinh<br />

2kBT<br />

with the summation i over all the phonon modes.<br />

From this partition function we obtain:<br />

Fvib kBT <br />

<br />

ˆi<br />

ln 2 sinh<br />

(3.17.4)<br />

2kBT<br />

i<br />

The energy º is assumed now to be a function of v only. Using (3.17.4) for<br />

Fvib we obtain an expression for P:<br />

<br />

dº<br />

P kBT<br />

dv<br />

<br />

<br />

ˆi dˆi<br />

coth<br />

(3.17.5)<br />

2kBT 2kBT dv<br />

i<br />

To simplify this expression we assume that the mode Grüneisen parameters<br />

for all the phonon modes are roughly the same and can be approximated by<br />

an average Grüneisen parameter 〈Á〉 ∼d(ln ˆi)/d(ln v) for all phonon modes.<br />

Within this approximation the expression for P simplifies to:<br />

<br />

dº 〈Á〉 <br />

<br />

ˆi ˆi<br />

P ≈ <br />

coth<br />

(3.17.6)<br />

dv v<br />

2kBT 2<br />

i<br />

i<br />

The average energy (like the average energy for photons) of a phonon mode<br />

with frequency ˆ is given by:<br />

U(ˆ) {n(1/2)}(ˆ) where n is the phonon occupancy or Bose-Einstein<br />

distribution function (see p. 126), given by: n [exp(ˆ/kBT)1] 1 . Using the<br />

result that {n (1/2)} (1/2) coth[(ˆ/2kBT)] we obtain:<br />

<br />

<br />

ˆi ˆi<br />

coth<br />

U (3.17.7)<br />

2kBT 2<br />

where U represents the internal energy of the crystal due to vibrational modes<br />

only. Hence we arrive at:<br />

P (dº/dv) 〈Á〉U/v (3.17.8)<br />

We can regard this relation between P and v as an equation-of-state of the<br />

crystal.<br />

Using this equation we can obtain the relation between the coefficient of<br />

thermal expansion ‚ and 〈Á〉 under a quasi-harmonic approximation. In this

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