context | $ w $ … grand canonical weight |
definiendum | $ \langle\hat N\rangle(\beta,\mu) := \sum_{N=0}^\infty w_N(\beta,\mu)\cdot N $ |
The notation “$\langle\hat N\rangle$” is chosen for the function because we can also introduce the sequence of observables $\hat N$ defined to give us the particle number of each canonical ensemble, i.e. $\hat N_N=N$, and then the above coincides with the proper grand canonical expectation value of $\hat N$. Notice that this $\hat N$ is sometimes denoted by $N$, which can get a little confusing.
$ \langle\hat N\rangle = - \frac{\partial}{\partial\mu}\Omega $ |
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$\frac{1}{\beta}\frac{\partial}{\partial\mu}\langle\hat N\rangle = \langle {\hat N}^2\rangle-\langle\hat N\rangle^2$ |
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