AREPO-RT: radiation hydrodynamics on a moving mesh

Kannan, Rahul; Vogelsberger, Mark; Marinacci, Federico; McKinnon, Ryan; Pakmor, Rüdiger; Springel, Volker

doi:10.1093/mnras/stz287

Title: AREPO-RT: radiation hydrodynamics on a moving mesh

Journal Article · 28 January 2019 · Monthly Notices of the Royal Astronomical Society

DOI: https://doi.org/10.1093/mnras/stz287 · OSTI ID:1495618

Kannan, Rahul ^[1]; Vogelsberger, Mark ^[2];

^[2];

^[3];

^[4]

Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States). Kavli Institute for Astrophysics and Space Research
Heidelberg Inst. for Theoretical Studies (Germany)
Heidelberg Inst. for Theoretical Studies (Germany); Zentrum fur Astronomie der Univ. at Heidelberg (Germany); Max-Planck-Inst. fur Astrophysik, Garching (Germany)

We introduce AREPO-RT, a novel radiation hydrodynamic (RHD) solver for the unstructured moving-mesh code AREPO. Our method solves the moment-based radiative transfer equations using the M1 closure relation. We achieve second-order convergence by using a slope-limited linear spatial extrapolation and a first-order time prediction step to obtain the values of the primitive variables on both sides of the cell interface. A Harten–Lax–van Leer flux function, suitably modified for moving meshes, is then used to solve the Riemann problem at the interface. The implementation is fully conservative and compatible with the individual time-stepping scheme of AREPO. It incorporates atomic hydrogen (H) and helium (He) thermochemistry, which is used to couple the ultraviolet radiation field to the gas. Additionally, infrared (IR) radiation is coupled to the gas under the assumption of local thermodynamic equilibrium between the gas and the dust. We successfully apply our code to a large number of test problems, including applications such as the expansion of HII regions, radiation pressure-driven outflows, and the levitation of optically thick layer of gas by trapped IR radiation. The new implementation is suitable for studying various important astrophysical phenomena, such as the effect of radiative feedback in driving galactic scale outflows, radiation-driven dusty winds in high-redshift quasars, or simulating the reionization history of the Universe in a self-consistent manner.

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Research Organization:: Krell Institute, Ames, IA (United States)

Sponsoring Organization:: USDOE Office of Science (SC); National Aeronautics and Space Administration (NASA); Alfred P. Sloan Foundation; Kavli Research Investment Fund; German Research Foundation (DFG); European Research Council (ERC)

Grant/Contract Number:: FG02-97ER25308; PF7-180163; NAS8-03060; NNX17AG29G; EXAGAL-308037; FG0297ER25308

OSTI ID:: 1495618

Alternate ID(s):: OSTI ID: 1610351

Journal Information:: Monthly Notices of the Royal Astronomical Society, Vol. 485, Issue 1; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 59 works

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