TY - JOUR
T1 - A radiation hydrodynamics scheme on adaptive meshes using the Variable Eddington Tensor (VET) closure
AU - Menon, Shyam H.
AU - Federrath, Christoph
AU - Krumholz, Mark R.
AU - Kuiper, Rolf
AU - Wibking, Benjamin D.
AU - Jung, Manuel
N1 - Publisher Copyright:
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union.
PY - 2020/6/30
Y1 - 2020/6/30
N2 - We present a new algorithm to solve the equations of radiation hydrodynamics (RHD) in a frequency-integrated, two-moment formulation. Novel features of the algorithm include i) the adoption of a non-local Variable Eddington Tensor (VET) closure for the radiation moment equations, computed with a ray-tracing method, ii) support for adaptive mesh refinement (AMR), iii) use of a time-implicit Godunov method for the hyperbolic transport of radiation, and iv) a fixed-point Picard iteration scheme to accurately handle the stiff nonlinear gas-radiation energy exchange. Tests demonstrate that our scheme works correctly, yields accurate rates of energy and momentum transfer between gas and radiation, and obtains the correct radiation field distribution even in situations where more commonly used - but less accurate - closure relations like the Flux-limited Diffusion and Moment-1 approximations fail. Our scheme presents an important step towards performing RHD simulations with increasing spatial and directional accuracy, effectively improving their predictive capabilities.
AB - We present a new algorithm to solve the equations of radiation hydrodynamics (RHD) in a frequency-integrated, two-moment formulation. Novel features of the algorithm include i) the adoption of a non-local Variable Eddington Tensor (VET) closure for the radiation moment equations, computed with a ray-tracing method, ii) support for adaptive mesh refinement (AMR), iii) use of a time-implicit Godunov method for the hyperbolic transport of radiation, and iv) a fixed-point Picard iteration scheme to accurately handle the stiff nonlinear gas-radiation energy exchange. Tests demonstrate that our scheme works correctly, yields accurate rates of energy and momentum transfer between gas and radiation, and obtains the correct radiation field distribution even in situations where more commonly used - but less accurate - closure relations like the Flux-limited Diffusion and Moment-1 approximations fail. Our scheme presents an important step towards performing RHD simulations with increasing spatial and directional accuracy, effectively improving their predictive capabilities.
KW - hydrodynamics
KW - methods: numerical
KW - radiation mechanisms: general
KW - radiative transfer
UR - http://www.scopus.com/inward/record.url?scp=85146924460&partnerID=8YFLogxK
U2 - 10.1017/S1743921322001429
DO - 10.1017/S1743921322001429
M3 - Article
SN - 1743-9213
VL - 16
SP - 358
EP - 364
JO - Proceedings of the International Astronomical Union
JF - Proceedings of the International Astronomical Union
ER -