Undergrad Is the Fermion number operator squared equal to itself?

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The discussion centers on whether the fermion number operator squared is equal to itself, specifically for fermionic states where the number of particles can only be 0 or 1. It is clarified that while the number operator applied to a specific fermionic state does equal its square, this is due to the properties of fermions and the Pauli exclusion principle. The mathematical reasoning shows that applying the number operator twice yields the same result as applying it once, confirming that ##\hat{n}^2 = \hat{n}## for fermionic states. Additionally, the exponential of the number operator is discussed, revealing that it simplifies under these conditions. The conversation concludes with a consensus on the operator's behavior and its implications in quantum mechanics.
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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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