Calculating The Fermi Energy - Condensed Matter Physics

In summary, to calculate the Fermi energy, EF, at 0K for potassium, we can use the equation EF = h2 √(3n) / 4m, where n is the number of atoms per unit volume and m is the atomic mass. To solve for n, we can use the equation n = N/v, where N is the total number of atoms and v is the volume. Using the given values for the atomic weight and density, we can solve for n and then plug it into the equation for EF to find the Fermi energy.
  • #1
12x4
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0

Homework Statement


Calculate the Fermi energy, EF at 0K for potassium (atomic weight = 39, density = 860 kgm3).

Homework Equations


KF3 = 3π2n
Fermi Momentum ρ = h(bar)KF

The Attempt at a Solution

:[/B]
For the first part:

Using: E = ρ2/ 2m
Can substitute Fermi momentum into that to get:

EF = h(bar)2 KF2 / 2m

KF2 = √(3π2n) = π√(3n)

Putting all the together I got:

EF = h(bar)2 π √(3n) / 2m

which is the same as: EF = h2 √(3n) / 4m

I'm not too sure what to do after this point as I'm not sure how the atomic weight or density can give me a value for n and m. I do have written in my notes that n = N/v but again I wasn't sure how this would help me. I feel like I must be going down the wrong path to come out with an equation that needs completely different things to what the question is providing me with. But honestly I have just started this condensed matter course and haven't really got my feet yet.Thanks in advance to anyone that replies.

 
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  • #2
12x4 said:
KF3 = 3π2n

KF2 = √(3π2n) = π√(3n)
You haven't solved for KF2 correctly. What do you get if you first solve for KF?
... I'm not sure how the atomic weight or density can give me a value for n and m. I do have written in my notes that n = N/v but again I wasn't sure how this would help me.

n is the number of atoms per unit volume, whereas mass density ρ is the mass per unit volume. Try to think of a way to relate n to ρ using the atomic mass, matom.
 
  • #3
Ooops yes not sure what i was thinking there. Thank you for your help i think I've cracked it now.
 

FAQ: Calculating The Fermi Energy - Condensed Matter Physics

What is the Fermi energy?

The Fermi energy is a concept in condensed matter physics that represents the energy level at which the highest occupied electron energy states in a material are located at absolute zero temperature.

Why is calculating the Fermi energy important?

Calculating the Fermi energy is important because it helps us understand the electronic properties of materials, such as their electrical conductivity and thermal conductivity. It also plays a crucial role in determining the behavior of electrons in a material, which is essential for understanding many physical phenomena.

How is the Fermi energy calculated?

The Fermi energy is calculated using the Fermi-Dirac distribution, which describes the probability of electrons occupying different energy states at a given temperature. The calculation involves integrating the distribution function over all energy states and solving for the value at which the integral is equal to the total number of electrons in the system.

What factors affect the value of the Fermi energy?

The value of the Fermi energy is affected by the number of electrons in the system, the density of states in the material, and the temperature. It also depends on the type of material and its electronic band structure.

Can the Fermi energy be experimentally measured?

Yes, the Fermi energy can be measured using various experimental techniques, such as photoemission spectroscopy, tunneling spectroscopy, and Hall effect measurements. These techniques involve directly measuring the energy of electrons in a material and comparing it to the calculated value of the Fermi energy.

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