An overview of methods for deriving the radiative transfer theory from the Maxwell equations. II: Approach based on the Dyson and Bethe-Salpeter equations

J Quant Spectrosc Radiat Transf. 2019 Feb:224:25-36. doi: 10.1016/j.jqsrt.2018.10.032. Epub 2018 Oct 23.

Abstract

In this paper, the vector radiative transfer equation is derived by means of the vector integral Foldy equations describing the electromagnetic scattering by a group of particles. By Assuming that in a discrete random medium the positions of the particles are statistically independent and by applying the Twersky approximation to the order-of-scattering expansion of the total field, we derive the Dyson equation for the coherent field and the ladder approximated Bethe-Salpeter equation for the dyadic correlation function. Then, under the far-field assumption for sparsely distributed particles, the Dyson equation is reduced to the Foldy integral equation for the coherent field, while the iterated solution of the Bethe-Salpeter equation ultimately yields the vector radiative transfer equation.

Keywords: Bethe–Salpeter equation; Discrete random media; Dyson equation; Electromagnetic scattering; Frequency-domain macroscopic electromagnetics; Radiative transfer theory.