Write and use the ordinary Euclidean Laplacian , so the generator of standard Brownian motion is half that operator. For a radial function , the Laplacian in polar coordinates is . With ,
Thus is a harmonic function on the punctured space.
We first justify that the singularity is not visited. For , stop at . The Itô formula makes a local martingale, and it is bounded on this annulus, hence a true martingale. The exit time is finite almost surely: by the Gaussian transition density. Taking the bounded terminal limit yields
If the origin were reached before , every smaller radius would first be reached, so letting shows that event has probability zero. Taking a countable sequence proves almost surely. Localization on increasing annuli now applies the Itô formula globally and gives the Bessel power local martingale
Stopping this continuous local martingale at any , including , preserves its local-martingale property.
For , the stopped path stays at radius at least , so . The bounded local martingale criterion makes it a true martingale. For , Brownian radial oscillations at its starting sphere give almost surely and the stopped process is constant. Thus the same true-martingale conclusion holds for .
For , the process is a strict local martingale. To prove this, write in distribution, with a standard -dimensional normal vector. For every shift ,
Indeed the integrand outside the unit ball is at most one, while inside it the Gaussian density is at most and the radial integral is a constant times . Brownian scaling therefore gives
A true martingale would have expectation at every time, which is impossible.
The printed range also permits , and this case must not be grouped with the bounded case. Here almost surely, by the same Gaussian bound for exit from a bounded ball. Moreover,
since the second expectation is at most . It too is a strict local martingale. The complete stopped inverse radial power martingale classification is therefore