Is the Fermion number operator squared equal to itself?

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Discussion Overview

The discussion revolves around the properties of the fermion number operator, particularly whether squaring the operator yields the same operator. Participants explore the implications of this property in the context of fermionic states, mathematical definitions, and operator algebra.

Discussion Character

  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants propose that acting on a fermionic state with the number operator squared behaves like acting with the number operator itself, suggesting a potential definition of ##\hat{n}^k = \hat{n}##.
  • Others argue that this cannot be true universally, as the expectation value of the number operator for a state with two particles would yield different results for the squared operator.
  • A later reply clarifies that for a specific fermionic state, the number operator can indeed equal its own square, as it can only yield values of 0 or 1.
  • One participant presents a series expansion for the exponential of the number operator, questioning the earlier simplifications and suggesting a correction involving the series for e.
  • Another participant discusses the implications of the Pauli exclusion principle on the number operator, illustrating how normal ordering affects the application of the squared operator on the vacuum state.
  • Further contributions explore the mathematical definitions and properties of the number operator, including its eigenvalues and their implications for squaring the operator.

Areas of Agreement / Disagreement

Participants express differing views on the properties of the fermion number operator, with no consensus reached on whether ##\hat{n}^2 = \hat{n}## universally applies or under what conditions it holds true.

Contextual Notes

The discussion includes various assumptions about the definitions of operators and their applications, particularly in relation to fermionic states and the implications of the Pauli exclusion principle. There are also unresolved mathematical steps in the derivations presented.

voila
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What the title says. Acting on a fermionic state with the number operator to a power is like acting with the fermionic operator itself. Does this allow us to define ## \hat{n}^k=\hat{n} ##? Or is there any picky mathematical reason not to do so?
 
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voila said:
What the title says. Acting on a fermionic state with the number operator to a power is like acting with the fermionic operator itself. Does this allow us to define ## \hat{n}^k=\hat{n} ##? Or is there any picky mathematical reason not to do so?

If you think about it for a second, you'll see that that can't possibly be true. The whole point of a number operator is that \langle \Psi|\hat{n}|\Psi\rangle gives the expected number of particles in state |\Psi\rangle. If |\Psi\rangle is a state with exactly two particles, then\langle \Psi|\hat{n}|\Psi\rangle = 2
\langle \Psi|(\hat{n})^2|\Psi\rangle = 4

[Edit]

I apologize. It depends on what you mean. Do you mean the number operator that gives the total number of particles (anywhere, in any state)? In that case, what I said is true.

However, for a specific state, there is a corresponding number operator, which counts the number of particles in that state. Since for Fermions, that has to be either 0 or 1, then you're right, the square will be 0 or 1, as well. So the number operator for a particular state is equal to its own square.
 
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Yup, I meant number operator for a fermionic state (number of particles equals either 0 or 1). So ##\exp({\hat{n}})=\sum{\frac{\hat{n}^k}{k!}}=\sum{\frac{\hat{n}}{k!}}=\hat{n}\sum{\frac{1}{k!}}=\hat{n} e ##?
 
voila said:
Yup, I meant number operator for a fermionic state (number of particles equals either 0 or 1). So ##\exp({\hat{n}})=\sum{\frac{\hat{n}^k}{k!}}=\sum{\frac{\hat{n}}{k!}}=\hat{n}\sum{\frac{1}{k!}}=\hat{n} e ##?

That's not quite right. I would say it's equal to (1 - \hat{n}) + e \hat{n}.
 
How come?
 
voila said:
How come?
Well e^{\hat{n}} = 1 + \hat{n} + \frac{1}{2} (\hat{n})^2 + \frac{1}{6} (\hat{n})^3 + .... But if \hat{n}^2 = \hat{n}, then this becomes:

Well e^{\hat{n}} = 1 + \hat{n} + \frac{1}{2} \hat{n} + \frac{1}{6} \hat{n} + ...
= 1 + \hat{n} (1 + \frac{1}{2} + \frac{1}{6} + ...)

But that series is the series for e-1. The series for e starts 1+1+1/2 + .... So

e^{\hat{n}} = 1 + \hat{n} (e-1)
 
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The fermion number operator is defined in terms of operators, c and c^\dagger, which destroy/create fermionic particles. Because of Pauli's exclusion principle, doubly applying any of those gives you zero, that is, c^2|0> = 0, and also (c^\dagger)(c^\dagger)|0>=0.

Now consider applying the square of the number operator onto the vacuum state, |0>. Since the number operator is defined as n=c^\dagger c, in this case we have

nn|0> = c^\dagger c c^\dagger c|0>

However, in order to produce meaningful answers the operators must be NORMAL ORDERED, that is, all the \daggers to the left. In doing this we end up with

nn|0> = c^\dagger c c^\dagger c|0>=c^\dagger (1-c^\dagger c) c|0> = c^\dagger c|0> - c^\dagger c^\dagger c c|0> = c^\dagger c|0> = n|0>

where we have used the fermionic anticommutation relations {c,c^\dagger}=1 and that cc|0>=0.
 
voila said:
Yup, I meant number operator for a fermionic state (number of particles equals either 0 or 1). So ##\exp({\hat{n}})=\sum{\frac{\hat{n}^k}{k!}}=\sum{\frac{\hat{n}}{k!}}=\hat{n}\sum{\frac{1}{k!}}=\hat{n} e ##?
You forgot the ##k=0## term.
 
Say we are in a box, so that ##\{\hat{C}(\vec{p},\sigma),\hat{C}^{\dagger}(\vec{p}',\sigma')\}=\delta_{\vec{p},\vec{p}'} \delta_{\sigma,\sigma'}## with the ##\delta##'s being Kronecker ##\delta##'s with values ##1## and ##0## rather than Dirac-##\delta## distributions. Then you can just do the calculation: By definition
$$\hat{N}=\hat{C}^{\dagger}(\vec{p},\sigma) \hat{C}(\vec{p},\sigma)$$
leading to
$$\hat{N}^2=\hat{C}^{\dagger} \hat{C} \hat{C}^{\dagger} \hat{C}=\hat{C}^{\dagger} [\{\hat{C},\hat{C}^{\dagger} \}-\hat{C^{\dagger} \hat{C}}] \hat{C}=\hat{C}^{\dagger} \hat{1} \hat{C}=\hat{N},$$
because ##\{C,C \}=2 \hat{C}^2=0##.

Another argument is that ##\hat{N}## has the eigenvalues 0 and 1, i.e.,
$$\hat{N}^2=\sum_{n=0}^1 |n \rangle \langle n|n^2 =\sum_{n=0}^1 |n \rangle \langle n|n=\hat{N},$$
because both ##0^2=0## and ##1^2=1##, i.e., for both eigenvalues ##n^2=n##.
 
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