Girvin, Yang Modern Condensed Matter Physics 2019 SSP · Problem 3.16

Lattices and Symmetries

Physics — Condensed Matter · cumulant-expansion

Problem

Consider a general probability distribution function of an arbitrary number of variables, and an observable AA that depends on these variables in an arbitrary way. We may always write ⟨eA⟩=eC,(3.69)\langle e^A \rangle = e^C, \tag{3.69} where CC is given by the so-called cumulant expansion C≡∑n=1∞1n!cn.(3.70)C \equiv \sum_{n=1}^{\infty} \frac{1}{n!} c_n. \tag{3.70} Without loss of generality, we may subtract a constant from AA to impose the constraint that ⟨A⟩=0\langle A \rangle = 0. Under this constraint show that the lowest few cumulants obey c1=0,c2=⟨A2⟩,c3=⟨A3⟩,c4=⟨A4⟩−3⟨A2⟩2.(3.71)\begin{aligned} c_1 &= 0, \tag{3.71} \\ c_2 &= \langle A^2 \rangle, \\ c_3 &= \langle A^3 \rangle, \\ c_4 &= \langle A^4 \rangle - 3\langle A^2 \rangle^2. \end{aligned} If the distribution of AA is close to Gaussian then we expect the cumulant series to converge rapidly.

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