Abstract. We describe an extension of the cosmological hydrodynamics code Enzo to include the self-consistent transport of ionizing radiation modeled in the flux-limited diffusion approximation. A novel feature of our algorithm is a coupled implicit solution of radiation transport, ionization kinetics, and gas photoheating, making the timestepping for this portion of the calculation resolution independent. The implicit system is coupled to the explicit cosmological hydrodynamics through operator splitting and solved with scalable multigrid methods. We summarize the numerical method, present a verification test on cosmological Strömgren spheres, and then apply it to the problem of cosmological hydrogen reionization
International audienceContext. Radiation controls the dynamics and energetics of many astrophysical ...
Context. Radiative transfer plays a crucial role in the star formation process. Because of the high ...
International audienceThe development of radiation hydrodynamical methods that are able to follow ga...
Radiation hydrodynamical transport of ionization fronts in the next generation of cosmological reion...
Aims. The transport of energy through radiation is very important in many astrophysical phenomena. I...
Aims. The transport of energy through radiation is very important in many astrophysical ph...
Aims. The importance of radiation to the physical structure of protoplanetary disks cannot be unders...
Aims. The importance of radiation to the physical structure of protoplanetary disks cannot be unders...
We explore the application of Monte Carlo transport methods to solving coupled radiation-hydrodynami...
International audienceContext. Radiative transfer has a strong impact on the collapse and the fragme...
We examine the epoch of hydrogen reionization using a new numerical method that allows us to self-co...
Context. Radiative transfer has a strong impact on the collapse and the fragmentation of prestellar ...
We present a new implementation of radiation hydrodynamics (RHD) in the adaptive mesh refinement (AM...
International audienceContext. Radiation controls the dynamics and energetics of many astrophysical ...
Context. Radiative transfer plays a crucial role in the star formation process. Because of the high ...
International audienceThe development of radiation hydrodynamical methods that are able to follow ga...
Radiation hydrodynamical transport of ionization fronts in the next generation of cosmological reion...
Aims. The transport of energy through radiation is very important in many astrophysical phenomena. I...
Aims. The transport of energy through radiation is very important in many astrophysical ph...
Aims. The importance of radiation to the physical structure of protoplanetary disks cannot be unders...
Aims. The importance of radiation to the physical structure of protoplanetary disks cannot be unders...
We explore the application of Monte Carlo transport methods to solving coupled radiation-hydrodynami...
International audienceContext. Radiative transfer has a strong impact on the collapse and the fragme...
We examine the epoch of hydrogen reionization using a new numerical method that allows us to self-co...
Context. Radiative transfer has a strong impact on the collapse and the fragmentation of prestellar ...
We present a new implementation of radiation hydrodynamics (RHD) in the adaptive mesh refinement (AM...
International audienceContext. Radiation controls the dynamics and energetics of many astrophysical ...
Context. Radiative transfer plays a crucial role in the star formation process. Because of the high ...
International audienceThe development of radiation hydrodynamical methods that are able to follow ga...