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Importance sampling, Fokker-Planck and Langevin equations

For very large t this becomes

\langle (\mathbf{r}(t)-\mathbf{r}_{0})^{2}\rangle =\frac{6kT}{m\xi }t

from which we get the Einstein relation

D= \frac{kT}{m\xi }

where we have used \langle (\mathbf{r}(t)-\mathbf{r}_{0})^{2}\rangle =6Dt .