Fermi energy condensed matter exam problem

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SUMMARY

The discussion centers on deriving the Fermi energy and Fermi wave number for a free electron gas at zero temperature. The Fermi energy is defined as ε_{F}=\frac{\hbar^{2}}{2m}(3π^{2}N)^{2/3} and the Fermi wave number as k_{F}=(3π^{2}N)^{1/3}, where N represents the volume density of electrons. Participants emphasize the importance of the density of states equation, D(ε) = \frac{V}{2π^{2}}(\frac{2m}{\hbar^{2}})^{3/2} ε^{1/2}, and discuss the correct order of derivation, with some suggesting that integrating the density of states from zero to the Fermi energy can yield the number of particles.

PREREQUISITES
  • Understanding of Fermi energy and Fermi wave number in condensed matter physics
  • Familiarity with the density of states equation in quantum mechanics
  • Knowledge of the dispersion relation for free electron gas, ε(k) = \frac{\hbar^{2}k^{2}}{2m}
  • Basic concepts of k-space and volume density of electrons
NEXT STEPS
  • Study the derivation of the density of states for a free electron gas
  • Learn about integrating the density of states to find particle numbers
  • Explore the implications of Fermi energy in different materials
  • Investigate the relationship between temperature and Fermi energy in electron gases
USEFUL FOR

Students preparing for condensed matter physics exams, physicists focusing on quantum mechanics, and researchers studying electronic properties of materials.

SMC
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Homework Statement



Hello, I am preparing a condensed matter exam and I was wondering if I could get some help on the following question from a past exam paper:

Show that for the free electron gas at zero temperature the Fermi energy is given by:

ε_{F}=\frac{\hbar^{2}}{2m}(3π^{2}N)^{2/3}

and the fermi wave number by:

k_{F}=(3π^{2}N)^{1/3}

where N is the volume density of electrons.

Homework Equations



the previous question was to derive the density of states:

D(ε) = \frac{V}{2π^{2}}(\frac{2m}{\hbar^{2}})^{3/2} ε^{1/2}

but I don't know if I have to use that or not

The Attempt at a Solution



how I would have done it is derive k_{F} from N=\frac{VK_{F}^{3}}{3π^{2}} which is obtained by saying number of electrons N is equal to volume of fermi sphere over k-space volume element (2π/L)^{3}.

and then state that the dispersion for a free electron gas is
ε(k) = \frac{\hbar^{2}k^{2}}{2m} to get fermi energy.

but this method gives a result with the V present in the equation while the equations in the question don't have the V for some reason. Also I derived wavenumber first then energy while the question asks to derive energy first then wavenumber.
 
Last edited:
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SMC - I think the N in the question is the number of particles per unit volume. Otherwise their equations aren't dimensionally correct.
 
yes ok that makes sense I should of noticed that, thank you Oxvillan. but I still don't understand why it asks me to derive fermi energy before wavenumber. is there a way of deriving fermi energy without deriving wavenumber first?

or maybe the questions are just in the wrong order
 
Actually I would have done the wavenumber first too :smile:

But you can also integrate the density of states in energy space from zero to whatever the Fermi energy is and set that equal to N.
 

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