Feynman Rules For Brownian Motion

We present a perturbation theory extending a prescription due to Feynman for computing the probability density function in Brownian-motion. The method used, can be applied to a wide variety of otherwise difficult circumstances in Brownian-motion. The exact moments and kurtosis, if not the distribution itself, for many important cases can be summed for arbitrary times. As expected, the behavior at early time regime, for the sample processes considered, deviate significantly from the usual diffusion theory; a fact with important consequences in various applications such as financial physics. A new class of functions dubbed "Damped-exponential-integrals" are also identified