Semi-implicit scheme for treating radiation under M1 closure in general relativistic conservative fluid dynamics codes

A numerical scheme is described for including radiation in multidimensional general relativistic conservative fluid dynamics codes. In this method, a covariant form of the M1 closure scheme is used to close the radiation moments, and the radiative source terms are treated semi-implicitly in order to handle both optically thin and optically thick regimes. The scheme has been implemented in a conservative general relativistic radiation hydrodynamics code koral. The robustness of the code is demonstrated on a number of test problems, including radiative relativistic shock tubes, static radiation pressure supported atmosphere, shadows, beams of light in curved space–time and radiative Bondi accretion. The advantages of M1 closure relative to other approaches such as the Eddington closure and flux-limited diffusion are discussed, and its limitations are also highlighted.