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 A that depends on these variables in an arbitrary way. We may always write
⟨eA⟩=eC,(3.69)
where C is given by the so-called cumulant expansion
C≡n=1∑∞n!1cn.(3.70)
Without loss of generality, we may subtract a constant from A to impose the constraint that ⟨A⟩=0. Under this constraint show that the lowest few cumulants obey
c1c2c3c4=0,=⟨A2⟩,=⟨A3⟩,=⟨A4⟩−3⟨A2⟩2.(3.71)
If the distribution of A is close to Gaussian then we expect the cumulant series to converge rapidly.