Radiation Transport for Explosive Outflows: A Multigroup Hybrid Monte Carlo Method
Ryan T. Wollaeger, Daniel R. van Rossum, Carlo Graziani, Sean M., Couch, George C. Jordan IV, Donald Q. Lamb, and Gregory A. Moses

TL;DR
This paper develops a multigroup hybrid Monte Carlo method combining IMC and DDMC for radiation transport in high-velocity outflows, with applications to supernovae and improved boundary conditions.
Contribution
It formulates a new high-velocity multigroup IMC-DDMC method with a novel boundary condition for photon transport in supernovae.
Findings
The new boundary condition is distinct from prior literature.
IMC-DDMC outperforms pure IMC in accuracy and speed with structured opacities.
The method is suitable for semi-relativistic radiation transport in fluids.
Abstract
We explore Implicit Monte Carlo (IMC) and Discrete Diffusion Monte Carlo (DDMC) for radiation transport in high-velocity outflows with structured opacity. The IMC method is a stochastic computational technique for nonlinear radiation transport. IMC is partially implicit in time and may suffer in efficiency when tracking Monte Carlo particles through optically thick materials. DDMC accelerates IMC in diffusive domains. Abdikamalov extended IMC and DDMC to multigroup, velocity-dependent transport with the intent of modeling neutrino dynamics in core-collapse supernovae. Densmore has also formulated a multifrequency extension to the originally grey DDMC method. We rigorously formulate IMC and DDMC over a high-velocity Lagrangian grid for possible application to photon transport in the post-explosion phase of Type Ia supernovae. This formulation includes an analysis that yields an…
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