Fermi Dirac distribution function

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Discussion Overview

The discussion revolves around the Fermi-Dirac distribution function, particularly its behavior at zero temperature and the implications of negative energy states in relation to the Fermi energy. Participants explore how the function behaves for negative energies, especially when the Fermi energy is positive, and the integration of the distribution function in specific contexts.

Discussion Character

  • Exploratory
  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant questions the behavior of the Fermi-Dirac distribution function, specifically f(-ε), when ε < ε_F and ε_F is not zero.
  • Another participant clarifies that states with energy less than the chemical potential are occupied with probability one, including negative energy states.
  • A participant notes that as T approaches 0, the Fermi function behaves like the Heaviside step function, indicating that the conditions reverse when substituting ε with -ε.
  • Further clarification is provided that the original question pertains to the behavior of the function for E < 0 when E_F > 0.
  • One participant shares their findings from plotting f(-ε), suggesting it is 1 for ε > -ε_F and 0 otherwise, and discusses the implications for integration involving the Fermi-Dirac functions.
  • A participant reminds others that the Hamiltonian is typically bounded from below, which affects the existence of states and thus the Fermi-Dirac function for energies below a certain threshold.
  • Another participant raises the point that the density of states can influence the occupation number, potentially causing it to vanish for ε < 0.

Areas of Agreement / Disagreement

Participants express varying interpretations of the Fermi-Dirac distribution function's behavior for negative energies, particularly in relation to the Fermi energy. There is no consensus on the implications of these behaviors, and multiple competing views remain regarding the integration and the role of the density of states.

Contextual Notes

Participants mention the dependence of the Fermi-Dirac function on the Hamiltonian's bounds and the density of states, which may affect the occupation of states at negative energies. These factors introduce limitations and conditions that are not fully resolved in the discussion.

Physicslad78
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I have a question that is puzzling me as always...The Fermi-Dirac distribution function is (at T=0):

f\epsilon=\frac{1}{e^{\beta(\epsilon-\epsilon_{F})}+1} and we know that we can subsitute f\epsilon by 1 for \epsilon< \epsilon_{F} and 0 otherwise. However what is f(-\epsilon)? The answer is easy when \epsilon_{F}=0 but what if \epsilon_{F} is not zero. what would be ff(-\epsilon)? for \epsilon< \epsilon_{F}?


Thanks
 
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Hi Physicslad78,

I'm a bit confused by your question. You state correctly that the Fermi function at zero temperature implies that any state with energy less than the chemical potential is occupied with probability one. This statement also applies to any negative energy states that may exist below the chemical potential. Is this what you were confused about?
 
As T \rightarrow 0,

f(\varepsilon) = \frac{1}{\exp\lrft[\beta(\varepsilon - \varepsilon_F)\right] + 1} \rightarrow \Theta(\varepsilon - \varepsilon_F),
which is the Heaviside step function, which is zero for e < e_F and 1 for e > e_F. If you replace e with -e, the equalities just get reversed: it's 0 for e > - e_F and 1 for e < -e_F.
 
Mute said:
If you replace e with -e, the equalities just get reversed: it's 0 for e > - e_F and 1 for e < -e_F.
If I understand the OP's question, this is not merely a question of a sign convention. Rather, it is asking what the function does for E<0, when E_F >0. That question is answered by Physics Monkey above.
 
Thanks guys for all of your replies.. What I wanted to know is that when does f (-\epsilon) vanish and when it is one. I guess Mute answered the question but he reversed the cases. i tried to plot f (-\epsilon) and found that is it is 1 for \epsilon>-\epsilon_{F} and 0 otherwise. The situation I am in is I am trying to integrate the following:

\int_{0}^{\infty}(f(\epsilon)-f(-\epsilon))(\frac{1}{\omega\hbar-2\epsilon}-\frac{1}{\omega\hbar+2\epsilon}. I want to know how the Fermi Dirac functions behave. If we divide the first integral into two: \int_{0}^{E_{F}+\int_{E_F}^{\infty} so that the first term gives an f(\epsilon) of 1 while the second vanishes..Now for f (-\epsilon), I think i can perform the change of variable x= -\epsilon so that dx= -d\epsilon and the integral limits now go from -\infty to 0 but now we can write - \int_{-\infty}^{0} is \int_{0}^{+\infty} which then also gives 1 so that the total would be 2 trimes the remaining functions to be integrated which will give Log i guess...Is that right??
 
Yes, probably, but you should keep in mind that your Hamiltonian is usually bounded from below, that is there is a minimal epsilon, which often is taken to be 0. For values of epsilon below, there is no FD function as there are no states to be occupied.
 
Isn't this just a matter of density of states? I mean, the Fermi-Dirac function covers the entire domain -∞ < ε < +∞, regardless. However, the density of states can, for instance, make the occupation number vanish for ε < 0, right?
 

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