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• W1979812345 endingPage "2231" @default.
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• W1979812345 abstract "We present a new implementation of radiation hydrodynamics (RHD) in the adaptive mesh refinement (AMR) code RAMSES. The multi-group radiative transfer (RT) is performed on the AMR grid with a first-order Godunov method using the M1 closure for the Eddington tensor, and is coupled to the hydrodynamics via non-equilibrium thermochemistry of hydrogen and helium. This moment-based approach has the large advantage that the computational cost is independent of the number of radiative sources - it can even deal with continuous regions of emission such as bound-free emission from gas. As it is built directly into RAMSES, the RT takes natural advantage of the refinement and parallelization strategies already in place. Since we use an explicit advection solver for the radiative transport, the time step is restricted by the speed of light - a severe limitation that can be alleviated using the so--called reduced speed of light approximation. We propose a rigorous framework to assess the validity of this approximation in various conditions encountered in cosmology and galaxy formation. We finally perform with our newly developed code a complete suite of RHD tests, comparing our results to other RHD codes. The tests demonstrate that our code performs very well and is ideally suited for exploring the effect of radiation on current scenarios of structure and galaxy formation." @default.
• W1979812345 created "2016-06-24" @default.
• W1979812345 creator A5021060545 @default.
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• W1979812345 date "2013-10-09" @default.
• W1979812345 modified "2023-10-13" @default.
• W1979812345 title "ramses-rt: radiation hydrodynamics in the cosmological context" @default.
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• W1979812345 doi "https://doi.org/10.1093/mnras/stt1722" @default.
• W1979812345 hasPublicationYear "2013" @default.
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