Stochastic-integral representation conjecture for the renormalised Amperean area

Let WW be the Brownian motion and let GG be the Green kernel appearing in the definition of the renormalised Amperean area. Write IWI_W for the recentred self-intersection local time, and interpret dWt{\rm d}\overleftarrow{W}_t as a backward stochastic integral. Stochastic-integral representation conjecture. The renormalised Amperean area A~W\tilde{\mathcal{A}}_W can be expressed as

AW=20Tˉ0sG(WsWt)dWtdWsIW/2\mathcal{A}_W=-2\int_0^{\bar{T}}\int_0^sG(W_s-W_t)\,{\rm d}\overleftarrow{W}_t\,{\rm d}W_s-I_W/2

and equivalently as

AW=20Tˉ0sG(WsWt)dWtdWs+IW/2.\mathcal{A}_W=-2\int_0^{\bar{T}}\int_0^sG(W_s-W_t)\,{\rm d}W_t\,{\rm d}W_s+I_W/2.

The counterterm needed to define AW\mathcal{A}_W is absorbed into the counterterm defining IWI_W. The corresponding Stratonovich integral is not known to be well-defined, although it may be defined as the average of the backward and forward integrals.

Sources & referencesView supporting material

Primary source

Isao Sauzedde, “Renormalised Amperean Area of Brownian Motions and Symanzik Representation of the 2D Abelian Yang–Mills–Higgs Field”, arXiv:2412.16781 (2024).

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