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On the transfer of resonant-line radiation in mesh simulations

2 Pith papers cite this work. Polarity classification is still indexing.

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abstract

The last decade has seen applications of Adaptive Mesh Refinement (AMR) methods for a wide range of problems from space physics to cosmology. With the advent of these methods, in which space is discretized into a mesh of many individual cubic elements, the contemporary analog of the extensively studied line radiative transfer (RT) in a semi-infinite slab is that of RT in a cube. In this study we provide an approximate solution of the RT equation, as well as analytic expressions for the probability distribution functions (pdfs) of the properties of photons emerging from a cube, and compare them with the corresponding slab problem. These pdfs can be used to perform fast resonant-line RT in optically thick AMR cells where, otherwise, it could take unrealistically long times to transfer even a handful of photons.

fields

astro-ph.GA 2

years

2026 2

verdicts

ACCEPT 2

representative citing papers

Force convergence in Monte Carlo Lyman-alpha radiative transfer

astro-ph.GA · 2026-07-09 · accept · novelty 6.0

A moment-based hierarchy (zeroth, first, second order) diagnoses convergence of Lyman-alpha MCRT momentum-transfer estimators, showing that core-skipping biases internal forces and that statistical precision, cost, and physical accuracy must be evaluated separately.

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