The last equation is very similar to the so-called Master equation, which relates the temporal dependence of a PDF wi(t) to various transition rates. The equation can be derived from the so-called Chapman-Einstein-Enskog-Kolmogorov equation. The equation is given as dwi(t)dt=∑j[W(j→i)wj−W(i→j)wi], which simply states that the rate at which the systems moves from a state j to a final state i (the first term on the right-hand side of the last equation) is balanced by the rate at which the system undergoes transitions from the state i to a state j (the second term). If we have reached the so-called steady state, then the temporal development is zero. This means that in equilibrium we have dwi(t)dt=0.