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Thermal fluctuations and response functions

Equilibrium thermodynamics describes average quantities, but microscopic systems continually fluctuate around those averages. Statistical mechanics relates the size of equilibrium fluctuations to macroscopic response functions.

In the canonical ensemble, $$\langle E\rangle=-\frac{\partial\ln Z}{\partial\beta}.$$ Differentiating again gives $$\operatorname{Var}(E)=\langle E^2\rangle-\langle E\rangle^2 =\frac{\partial^2\ln Z}{\partial\beta^2}.$$ Using $\beta=1/(k_BT)$ and $$C_V=\left(\frac{\partial\langle E\rangle}{\partial T}\right)_V,$$ one obtains $$\operatorname{Var}(E)=k_BT^2C_V.$$ Thus a system with larger heat capacity exhibits larger absolute energy fluctuations at the same temperature.

For an extensive system, both $\langle E\rangle$ and $C_V$ typically scale with particle number $N$. The standard deviation therefore scales as $\sqrt N$ while the mean scales as $N$, so relative fluctuations behave roughly as $$\frac{\sigma_E}{\langle E\rangle}\sim\frac{1}{\sqrt N}.$$ This explains why macroscopic thermodynamic variables appear effectively deterministic despite microscopic fluctuations.

Similar fluctuation-response relations connect particle-number fluctuations to compressibility and magnetization fluctuations to magnetic susceptibility. The broader lesson is that response and noise are two sides of equilibrium statistical behavior: how strongly a system fluctuates encodes how strongly it responds to an applied thermodynamic field.