Average Kinetic Energy of Electron in the Conduction Band

Click For Summary
SUMMARY

The average kinetic energy (K.E.) of electrons in the conduction band can be expressed as <K.E.> = E_c + (3/2)k_B T. This expression is derived from the integral <K.E.> = (∫ (E - E_c) g(E) f(E) dE) / (∫ g(E) f(E) dE), where g(E) is the density of states and f(E) is the Fermi-Dirac distribution. The integration process involves substituting x = (E - E_c) / (k_B T) and applying the Feynman-Hellmann theorem to simplify the numerator and denominator integrals.

PREREQUISITES
  • Understanding of solid state physics concepts
  • Familiarity with statistical mechanics and the Fermi-Dirac distribution
  • Knowledge of integration techniques in calculus
  • Proficiency in using the Feynman-Hellmann theorem
NEXT STEPS
  • Study the derivation of the Fermi-Dirac distribution in detail
  • Learn about the density of states in solid state physics
  • Explore applications of the Feynman-Hellmann theorem in statistical mechanics
  • Practice integration techniques involving exponential functions and polynomial terms
USEFUL FOR

Physicists, materials scientists, and students studying solid state physics or statistical mechanics who are interested in understanding electron behavior in conduction bands.

Teymur
Messages
16
Reaction score
3
Homework Statement
Show that:
$$<\:K.E.>\:=E_c+3/2\:k_B\:T$$
Relevant Equations
$$<\:K.E.>\:=\frac{\left(total\:K.E.\right)}{\left(no.of\:electrons\right)}$$

$$<\:K.E.>\:=\:\frac{\int \:\left(E-E_c\right)g\left(E\right)f\left(E\right)dE}{\int \:g\left(E\right)f\left(E\right)dE}$$
Hello,
I've seen in a few books on solid state physics that one can deduce an expression for average K.E.:

$$<\:K.E.>\:=E_c+3/2\:k_B\:T$$

from the following:

$$<\:K.E.>\:=\:\frac{\int \:\left(E-E_c\right)g\left(E\right)f\left(E\right)dE}{\int \:g\left(E\right)f\left(E\right)dE}$$

I can't, however, find any work through of how to do so. I've had a go at the bottom part:

where ##n=\int g\left(E\right)f\left(E\right)dE## and ##\int \:x^{\frac{1}{2}}exp\left(-x\right)dx=\frac{\pi \:^{\frac{1}{2}}}{2}##

and

##g\left(E\right)=\frac{\left(2m_e\right)^{\frac{3}{2}}\left(E-E_c\right)^{\frac{1}{2}}}{2\pi ^2ℏ^3}## and ##f\left(E\right)\approx exp\left(\frac{\mu -E}{k_B\:T}\right)##

to get:

$$n=2\left(\frac{m_ek_B\:T}{2\pi ℏ^2}\right)^{\frac{3}{2}}\:exp\left(\frac{\mu -E_c}{k_B\:T}\right)$$

But how does one integrate the numerator with the ##\left(E\:-E_c\right)## term and simplify to the desired result?
 
Physics news on Phys.org
p.s. I used: ##x=\left(\frac{E-E_c}{k_B\:T}\right)## for the integral: ##\int \:g\left(E\right)f\left(E\right)dE \rightarrow \int \:x^{\frac{1}{2}}exp\left(-x\right)dx##
 
Teymur said:
But how does one integrate the numerator with the ##\left(E\:-E_c\right)## term and simplify to the desired result?
The numerator integration is very similar to the integration in the denominator. The factor ##\left(E\:-E_c\right)## has a simple relation to ##x##.
 
  • Like
Likes   Reactions: PeroK and hutchphd
Aha .. I'm not sure why I didn't spot that.
 
Another very important trick used in statistical physics is to calculate the denominator, the socalled "partition sum" and then take a derivative wrt. ##\beta=1/(k_{\text{B}} T)##, which is an application of the celebrated Feynman-Hellmann theorem.
 
  • Like
Likes   Reactions: PeroK

Similar threads

  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 0 ·
Replies
0
Views
2K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 10 ·
Replies
10
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 7 ·
Replies
7
Views
3K
Replies
4
Views
742
Replies
19
Views
3K