A quick question about the Fermi-Dirac distribution

In summary: The electrons interact weakly with each other (via the Pauli exclusion principle) but do not feel the nucleus (due to the approximation of neglecting electron-electron interaction and the fact that the nucleus is very heavy).In summary, The Fermi-Dirac distribution describes the probability for each single-particle state occupied by an electron. When taking into account degeneracy, the mean number of electrons in a given energy level will be twice the value given by the distribution. At temperatures close to 0K, the lowest N/2 states of an atom will be occupied, with N/2 electrons in spin up states and N/2 in spin down states. The term "single-particle state" refers to a state in which
  • #1
davon806
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Homework Statement


An electron has two spin states and a set of energy levels E1,E2,...
By the Fermi-dirac distrbution,the mean number of electrons in energy level Ek is
https://en.wikipedia.org/wiki/Fermi–Dirac_statistics#Distribution_of_particles_over_energy
Does it mean that,for an electron, the mean number is 2*F(E) ? But this sounds weird to me,because the mean number doubles just because of the degeneracy ? I am quite confused.

*Additional
If we take degeneracy into account,suppose there are N electrons(weakly-interacting).At some temperatures close to 0K,the N/2 states of lowest energy are occupied rather than N states?

Homework Equations

The Attempt at a Solution


Described in 1.
 
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  • #2
The probability for each state is given by the distribution. If you sum over two states (e. g. two spin states), the mean number of electrons will be twice that value, sure.
davon806 said:
If we take degeneracy into account,suppose there are N electrons(weakly-interacting).At some temperatures close to 0K,the N/2 states of lowest energy are occupied rather than N states?
The lowest N states are occupied, N/2 of them will be spin up, N/2 will be spin down (neglecting couplings between spin and anything else).
 
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  • #3
mfb said:
The probability for each state is given by the distribution. If you sum over two states (e. g. two spin states), the mean number of electrons will be twice that value, sure.
The lowest N states are occupied, N/2 of them will be spin up, N/2 will be spin down (neglecting couplings between spin and anything else).
But for each state, can we accommodate 2 electrons? 1 with spin up and 1 with spin down,so that eventually the lowest N/2 states will be occupied?
 
  • #4
davon806 said:
But for each state, can we accommodate 2 electrons? 1 with spin up and 1 with spin down,so that eventually the lowest N/2 states will be occupied?
It depends how you define the state. @mfb is using state to mean unique single-particle states, including spin (so there is no degeneracy factor appearing). You seem to mean state being an energy state, a state defined only by the its energy, which can be degenerate due to spin.

Both approaches are valid, but you have to be clear what you are considering.
 
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  • #5
DrClaude said:
It depends how you define the state. @mfb is using state to mean unique single-particle states, including spin (so there is no degeneracy factor appearing). You seem to mean state being an energy state, a state defined only by the its energy, which can be degenerate due to spin.

Both approaches are valid, but you have to be clear what you are considering.

Could you explain what's meant by a single-particle state?This term comes up in my notes frequently but I have no idea what it is referring to?:nb)
 
  • #6
davon806 said:
Could you explain what's meant by a single-particle state?
It is a state in which a single-particle can fit :wink:

Let me take an atom as an example. If you solve the (non-relativistic) Schrödinger equation for a hydrogenic atom (1 electron, charge of the nucleus ≥ 1), you will find a series of eigenstates, which can be characterized by the quantum numbers ##n,l,m## and ##m_s##. Each valid combination of these quantum numbers gives you one single-particle state.

The full state of an atom, while neglecting electron-electron interaction, would correspond to putting a series of electrons in these single-particle states, with at most one electron in each (Pauli exclusion principle).
 
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1. What is the Fermi-Dirac distribution?

The Fermi-Dirac distribution is a probability distribution that describes the distribution of particles in a quantum system at thermal equilibrium. It was developed by Enrico Fermi and Paul Dirac to explain the behavior of fermions, which are particles with half-integer spin.

2. How is the Fermi-Dirac distribution different from the Maxwell-Boltzmann distribution?

The main difference between the Fermi-Dirac distribution and the Maxwell-Boltzmann distribution is that the former takes into account the principle of exclusion, which states that no two fermions can occupy the same energy state. This results in a more gradual decrease in the probability of occupying higher energy states, compared to the sharp decline in the Maxwell-Boltzmann distribution.

3. What is the significance of the Fermi level in the Fermi-Dirac distribution?

The Fermi level, also known as the chemical potential, is the energy level at which the probability of finding a particle is equal to 0.5. It is a crucial parameter in the Fermi-Dirac distribution as it determines the average energy and number of particles in a system at thermal equilibrium.

4. How does temperature affect the Fermi-Dirac distribution?

Increasing the temperature of a system described by the Fermi-Dirac distribution will result in a broader distribution with a higher average energy. This is because at higher temperatures, more energy states become available for fermions to occupy, and the probability of occupying higher energy states increases.

5. What are some real-world applications of the Fermi-Dirac distribution?

The Fermi-Dirac distribution has numerous applications in physics and engineering, including understanding the behavior of electrons in materials, such as semiconductors and metals. It is also used in the study of degenerate matter, such as white dwarfs and neutron stars, and plays a crucial role in the calculation of electronic and thermal properties of materials.

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