AREPO-RT: radiation hydrodynamics on a moving mesh
Abstract
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 dustymore »
- Authors:
-
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, 02138 MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Ave, Cambridge, 02139 MA, USA
- Heidelberg Institute for Theoretical Studies, Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany
- Heidelberg Institute for Theoretical Studies, Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany, Zentrum für Astronomie der Universität Heidelberg, ARI, Mnchhof-str. 12-14, D-69120 Heidelberg, Germany, Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85741 Garching, Germany
- Publication Date:
- Research Org.:
- Krell Institute, Ames, IA (United States)
- Sponsoring Org.:
- 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)
- OSTI Identifier:
- 1495618
- Alternate Identifier(s):
- OSTI ID: 1610351
- Grant/Contract Number:
- FG0297ER25308; FG02-97ER25308; PF7-180163; NAS8-03060; NNX17AG29G; EXAGAL-308037
- Resource Type:
- Published Article
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 485 Journal Issue: 1; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United Kingdom
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; astronomy & astrophysics; radiative transfer; radiation: dynamics; methods: numerical
Citation Formats
Kannan, Rahul, Vogelsberger, Mark, Marinacci, Federico, McKinnon, Ryan, Pakmor, Rüdiger, and Springel, Volker. AREPO-RT: radiation hydrodynamics on a moving mesh. United Kingdom: N. p., 2019.
Web. doi:10.1093/mnras/stz287.
Kannan, Rahul, Vogelsberger, Mark, Marinacci, Federico, McKinnon, Ryan, Pakmor, Rüdiger, & Springel, Volker. AREPO-RT: radiation hydrodynamics on a moving mesh. United Kingdom. https://doi.org/10.1093/mnras/stz287
Kannan, Rahul, Vogelsberger, Mark, Marinacci, Federico, McKinnon, Ryan, Pakmor, Rüdiger, and Springel, Volker. Mon .
"AREPO-RT: radiation hydrodynamics on a moving mesh". United Kingdom. https://doi.org/10.1093/mnras/stz287.
@article{osti_1495618,
title = {AREPO-RT: radiation hydrodynamics on a moving mesh},
author = {Kannan, Rahul and Vogelsberger, Mark and Marinacci, Federico and McKinnon, Ryan and Pakmor, Rüdiger and Springel, Volker},
abstractNote = {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.},
doi = {10.1093/mnras/stz287},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 1,
volume = 485,
place = {United Kingdom},
year = {2019},
month = {1}
}
https://doi.org/10.1093/mnras/stz287
Web of Science
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Works referencing / citing this record:
Local photoionization feedback effects on galaxies
journal, September 2019
- Obreja, Aura; Macciò, Andrea V.; Moster, Benjamin
- Monthly Notices of the Royal Astronomical Society, Vol. 490, Issue 2