Force convergence in Monte Carlo Lyman-alpha radiative transfer
Joshua Kasiri, Aaron Smith, Kevin Lorinc, Olof Nebrin, Kazutaka Kimura
UT Dallas · UT Dallas · UT Dallas · Stockholm · Tohoku
astro-ph.GA
Submitted: 2026-07-09
Comments: 22 pages, 15 figures. Comments welcomed
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- THOR: a GPU-accelerated and MPI-parallel radiative transfer code
- Analytical and fitting formulae for solutions to Lyman-alpha radiative transfer equations: the effects of geometry, recoil, and velocity gradients
- Core-wing transitions and the breakdown of diffusion in Lyman-$\alpha$ radiative transfer
- Lyman-$\alpha$ radiation pressure regulates star formation efficiency
- Modelling the nebular emission of galaxies across cosmic time with COLT
- Lyman-alpha Radiation Pressure in Dense Star Clusters: Implications for Star Formation and Winds at Cosmic Dawn
- Lyman-alpha Pressure Strongly Enhances Pre-Supernova Feedback at Cosmic Dawn: The First Multi-Dimensional Lyman-alpha Radiation Hydrodynamics Simulations
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