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arxiv: 1612.03440 · v1 · pith:ELAEKQ2Knew · submitted 2016-12-11 · 🌌 astro-ph.SR

A Note on the Radiative and Collisional Branching Ratios in Polarized Radiation Transport with Coherent Scattering

classification 🌌 astro-ph.SR
keywords varepsilontinybranchingcoherentemissivityradiationratioscollisional
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We discuss the implementation of physically meaningful branching ratios between the CRD and PRD contributions to the emissivity of a polarized multi-term atom in the presence of both inelastic and elastic collisions. Our derivation is based on a recent theoretical formulation of partially coherent scattering, and it relies on a heuristic diagrammatic analysis of the various radiative and collisional processes to determine the proper form of the branching ratios. The expression we obtain for the emissivity is $\varepsilon=\left[\varepsilon^{\tiny (1)}-\varepsilon^{\tiny (2)}_{\rm f.s.} \right]+\varepsilon^{\tiny (2)}$, where $\varepsilon^{\tiny (1)}$ and $\varepsilon^{\tiny (2)}$ are the emissivity terms for the redistributed and partially coherent radiation, respectively, and where "f.s." implies that the corresponding term must be evaluated assuming a flat-spectrum average of the incident radiation.

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