+Octo-TIGER is an adaptive, octree-based code for modeling self-gravitating hydrodynamics in interacting binaries. We have extended Octo-TIGER to include gray radiation transport via the M1 moment method, coupling radiation energy and flux to the existing PPM hydrodynamics and FMM gravity solvers within a task-based HPX framework. Radiation variables are discretized on the same AMR mesh and evolved using an implicit-explicit scheme to handle both optically thick and thin regimes while conserving total energy and radiative flux. We validate the RHD module with standard radiation test problems, including a planar radiation front propagating through uniform media, radiative equilibration in matter–radiation coupling tests, and diffusion of a Gaussian radiation pulse. These benchmarks confirm the accuracy and efficiency of the M1 implementation in Octo-TIGER, laying the groundwork for forthcoming production runs of interacting binaries with full radiation feedback.
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