On spider diffusions having a spinning measure selected from their own local time
Isaac Ohavi, Miguel Martinez
TL;DR
The paper advances Walsh's spider diffusion theory by allowing the spinning measure to depend on the process's own local time at the junction, and develops a comprehensive framework encompassing an Itô formula, absolute continuity, Feynman-Kac representations for local-time Kirchhoff problems, quadratic local-time approximations, strong Markov properties, and diffusion scattering at the vertex. The approach unifies stochastic martingale problems with PDEs on networks, yielding probabilistic representations for backward parabolic systems and rigorous analysis of density and non-atomic behavior at the junction. The results collectively extend previous constant-spinning-measure theories to non-constant, time- and local-time-dependent regimes, with potential implications for stochastic scattering control and boundary conditions on graph-like domains. The work provides a robust toolkit for analyzing star-shaped network diffusions with locally time-driven boundary behavior and offers precise asymptotics for scattering distributions in terms of the dynamic spinning coefficients $\alpha_i(t,l)$.
Abstract
The aim of this article is to give several results related to Walsh's spider diffusions living on a star-shaped network that have a spinning measure selected from the own local time of the motion at the vertex (cf.[17]). We prove the corresponding Itô's formula and give some global trajectory properties such as $L^1$-approximation of the local time and the Markov property. Regarding the behavior of the process at the vertex, we show that that the distribution of the process is non atomic at the junction point and we characterize the instantaneous scattering distribution along some ray with the aid of the probability coefficients of diffraction. We obtain also a Feynmann-Kac representation for linear parabolic systems posed on star-shaped networks that where introduced in [18] possessing a so-called local-time Kirchhoff's boundary condition.
