I'm a physics master student and I have difficulties understanding how to derive the Fokker Planck equation from the Stratonovich SDE.
With the Ito SDE it is simple since the noise is independent of $X_t$ :
- With a physics notation :
$\dot{X} = \mu(X,t)+\sigma(X,t)\xi(t) $ with $\langle\xi(t)\rangle=0$ and $\langle\xi(t)\xi(s)\rangle = 2B\delta(t-s) $
Which can be written rigorously : $X_t = \mu(X_t,t)dt+\sigma(X_t,t)\sqrt{2B}dB_t$
- Then one takes an arbitrary function f with the right properties ($\mathcal{C}^2$, compactly supported etc.) and evaluates the expected value of $f(X_t)$ to derive the F.-P. equation :
$\frac{d\langle f(X(t)\rangle}{dt} = \langle f'(X)\dot{X}+B\sigma(X,t)^2f''(X)\rangle$
$\frac{d\langle f(X(t)\rangle}{dt} = \langle f'(X)\mu(X,t)+B\sigma(X,t)^2f''(X)\rangle+0$ since $\langle f(X)\sigma(X,t)\xi(t)\rangle=0$
- Finally a simple integration by part enables you to get :
$\int f(x) \partial_t p(x,t) dx = \int f(x) \partial_x\left( -\mu(x,t)p(x,t) + B\partial_x(\sigma(x,t)^2p(x,t))\right) \implies \partial_t p(x,t)=\partial_x\left( -\mu(x,t)p(x,t) + B\partial_x(\sigma(x,t)^2p(x,t))\right)$
If we consider the same problem with a Stratonovich approach:
$\frac{d\langle f(X(t)\rangle }{dt} = \langle f'(X)\dot{X}\rangle= \langle f'(X)\left( \mu(X,t)+\sigma(X,t)\xi(t) \right)\rangle$
But $\langle f'(X)\sigma(X,t)\xi(t)\rangle \neq 0$
How do we get from here to the Stratonovich Fokker-Planck equation ?