Misc,

Discrete diffusion Lyman-alpha radiative transfer

, , , and .
(2017)cite arxiv:1709.10187Comment: 13 pages, 12 figures, MNRAS, submitted.

Abstract

Due to its accuracy and generality, Monte Carlo radiative transfer (MCRT) has emerged as the prevalent method for Ly$\alpha$ radiative transfer in arbitrary geometries. The standard MCRT encounters a significant efficiency barrier in the high optical depth, diffusion regime. Multiple acceleration schemes have been developed to improve the efficiency of MCRT but the noise from photon packet discretization remains a challenge. The discrete diffusion Monte Carlo (DDMC) scheme has been successfully applied in state-of-the-art radiation hydrodynamics (RHD) simulations. Still, the established framework is not optimal for resonant line transfer. Inspired by the DDMC paradigm, we present a novel extension to resonant DDMC in which diffusion in space and frequency are treated on equal footing. We explore the robustness of our new method and demonstrate a level of performance that justifies incorporating the method into existing Ly$\alpha$ codes. We present computational speedups of $\sim 10^2$-$10^6$ relative to contemporary MCRT implementations with aggressive core-skipping. This is because the resonant DDMC runtime scales with the spatial and frequency resolution rather than the number of scatterings - the latter is typically $\tau_0$ for static media, or $(a \tau_0)^2/3$ with core-skipping. We anticipate new frontiers in which on-the-fly Ly$\alpha$ radiative transfer calculations are feasible in 3D RHD. More generally, resonant DDMC is transferable to any computationally demanding problem amenable to a Fokker-Planck approximation of frequency redistribution.

Tags

Users

  • @miki

Comments and Reviews