A Godunov Method for Multidimensional Radiation Magnetohydrodynamics based on a variable Eddington tensor
arXiv:1201.2223 · doi:10.1088/0067-0049/199/1/14
Abstract
We describe a numerical algorithm to integrate the equations of radiation magnetohydrodynamics in multidimensions using Godunov methods. This algorithm solves the radiation moment equations in the mixed frame, without invoking any diffusion-like approximations. The moment equations are closed using a variable Eddington tensor whose components are calculated from a formal solution of the transfer equation at a large number of angles using the method of short characteristics. We use a comprehensive test suite to verify the algorithm, including convergence tests of radiation-modified linear acoustic and magnetosonic waves, the structure of radiation modified shocks, and two-dimensional tests of photon bubble instability and the ablation of dense clouds by an intense radiation field. These tests cover a very wide range of regimes, including both optically thick and thin flows, and ratios of the radiation to gas pressure of at least 10^{-4} to 10^{4}. Across most of the parameter space, we find the method is accurate. However, the tests also reveal there are regimes where the method needs improvement, for example when both the radiation pressure and absorption opacity are very large. We suggest modifications to the algorithm that will improve accuracy in this case. We discuss the advantages of this method over those based on flux-limited diffusion. In particular, we find the method is not only substantially more accurate, but often no more expensive than the diffusion approximation for our intended applications.
42 pages, 22 figures, 2 tables, accepted by ApJS
References in corpus (7)
- Theory of Star Formation
- Athena: A New Code for Astrophysical MHD
- Theory of Core-Collapse Supernovae
- The RAGE radiation-hydrodynamic code
- The Effects of Radiative Transfer on Low-Mass Star Formation
- Equations and Algorithms for Mixed Frame Flux-Limited Diffusion Radiation Hydrodynamics
- Star Formation in Quasar Disk
Cited by in corpus (89)
- The Athena++ Adaptive Mesh Refinement Framework: Design and Magnetohydrodynamic Solvers
- Dedalus: A Flexible Framework for Numerical Simulations with Spectral Methods
- A Global Three Dimensional Radiation Magneto-hydrodynamic Simulation of Super-Eddington Accretion Disks
- Numerical simulations of super-critical black hole accretion flows in general relativity
- Three-Dimensional General Relativistic Radiation Magnetohydrodynamical Simulation of Super-Eddington Accretion, using a new code HARMRAD with M1 Closure
- Super-Eddington Accretion Disks around Supermassive black Holes
- Three-dimensional simulations of super-critical black hole accretion disks --- luminosities, photon trapping and variability
- A scheme for radiation pressure and photon diffusion with the M1 closure in RAMSES-RT
- Global simulations of axisymmetric radiative black hole accretion disks in general relativity with a sub-grid magnetic dynamo
- Semi-implicit scheme for treating radiation under M1 closure in general relativistic conservative fluid dynamics codes
- Dynamics of Dusty Radiation Pressure Driven Shells and Clouds: Fast Outflows from Galaxies, Star Clusters, Massive Stars, and AGN
- Local Radiation Hydrodynamic Simulations of Massive Star Envelopes at the Iron Opacity Peak
- A new multidimensional, energy-dependent two-moment transport code for neutrino-hydrodynamics
- Prompt Radiation and Mass Outflows from the Stream-Stream Collisions of Tidal Disruption Events
- Magnetohydrodynamic Simulations of Active Galactic Nucleus Disks and Jets
- Evolution of Accretion Disks in Tidal Disruption Events
- On the Thermal Stability of Radiation Dominated Accretion Disks
- A Two-moment Radiation Hydrodynamics Module in Athena Using a Time-explicit Godunov Method
- X-ray Spectra from MHD Simulations of Accreting Black Holes
- An Algorithm for Radiation Magnetohydrodynamics Based on Solving the Time-dependent Transfer Equation
- A New Numerical Scheme for Cosmic Ray Transport
- Monte Carlo Radiative Transfer
- Outflows Driven by Quasars in High-Redshift Galaxies with Radiation Hydrodynamics
- Spectra of Black Hole Accretion Models of Ultra-Luminous X-ray Sources
- Radiation Magnetohydrodynamics In Global Simulations Of Protoplanetary Disks
- Iron Opacity Bump Changes the Stability and Structure of Accretion Disks in Active Galactic Nuclei
- Radiation Feedback in ULIRGS: Are Photons Movers and Shakers?
- Global Hydromagnetic Simulations of Protoplanetary Disks with Stellar Irradiation and Simplified Thermochemistry
- Monte Carlo Radiation Hydrodynamics with Implicit Methods
- Numerical Simulations of Optically Thick Accretion onto a Black Hole - II. Rotating Flow
- Radiation Magneto-hydrodynamic Simulations of the Formation of Hot Accretion Disk Coronae
- An Implicit Finite Volume Scheme to Solve the Time Dependent Radiation Transport Equation Based on Discrete Ordinates
- Radiation-driven outflows from and radiative support in dusty tori of active galactic nuclei
- Radiation hydrodynamics integrated in the code PLUTO
- Astrophysics of Super-massive Black Hole Mergers
- HEROIC: 3D General Relativistic Radiative Postprocessor with Comptonization for Black Hole Accretion Discs
- Hybrid Adaptive Ray-Moment Method (HARM): A Highly Parallel Method for Radiation Hydrodynamics on Adaptive Grids
- Direct Collapse to Supermassive Black Hole Seeds with Radiative Transfer: Isolated Halos
- Radiation Hydrodynamic Simulations of Dust-Driven Winds
- Saturation of the MRI in Strongly Radiation Dominated Accretion Disks
- Cloud Formation and Acceleration in a Radiative Environment
- DISPATCH: A Numerical Simulation Framework for the Exa-scale Era. I. Fundamentals
- Neutrino fast flavor oscillations with moments: linear stability analysis and application to neutron star mergers
- Non-linear Evolution of Rayleigh-Taylor Instability in a Radiation Supported Atmosphere
- Dusty Cloud Acceleration by Radiation Pressure in Rapidly Star-Forming Galaxies
- The effects of irradiation on the cloud evolution in active galactic nuclei
- Resolution Requirements and Resolution Problems in Simulations of Radiative Feedback in Dusty Gas
- Quokka: A code for two-moment AMR radiation hydrodynamics on GPUs
- Multi-Frequency General Relativistic Radiation-Hydrodynamics with Closure
- Radiation-Hydrodynamics with MPI-AMRVAC: Flux-Limited Diffusion
- The Athena++ Adaptive Mesh Refinement Framework: Multigrid Solvers for Self-Gravity
- A two-moment radiation hydrodynamics scheme applicable to simulations of planet formation in circumstellar disks
- Radiation Hydrodynamics using Characteristics on Adaptive Decomposed Domains for Massively Parallel Star Formation Simulations
- Arepo-MCRT: Monte Carlo Radiation Hydrodynamics on a Moving Mesh
- MOCMC: Method of Characteristics Moment Closure, a Numerical Method for Covariant Radiation Magnetohydrodynamics
- Radiation hydrodynamics including irradiation and adaptive mesh refinement with AZEuS. I. Methods
- The Effects of Magnetic Fields on the Dynamics of Radiation Pressure Dominated Massive Star Envelopes
- A Family of Independent Variable Eddington Factor Methods with Efficient Preconditioned Iterative Solvers
- Radiation transport methods in star formation simulations
- Time Dependent Radiation Hydrodynamics on a Moving Mesh
- Smoothed Particle Radiation Hydrodynamics: Two-Moment method with Local Eddington Tensor Closure
- Thermal Stability in Turbulently Mixed Accretion Discs
- Effects of local dissipation profiles on magnetized accretion disk spectra
- Three Dimensional Natures of Massive Star Envelopes
- Synthesizing Spectra from 3D Radiation Hydrodynamic Models of Massive Stars Using Monte Carlo Radiation Transport
- Toward realistic simulations of magneto-thermal winds from weakly-ionized protoplanetary disks
- CAFE-R a code that solves the special relativistic radiation hydrodynamics equations
- A New Discrete Implicit Monte Carlo Scheme for Simulating Radiative Transfer Problems
- Thermal instability in radiation hydrodynamics: instability mechanisms, position-dependent S-curves, and attenuation curves
- An Asymptotically-Correct Implicit-Explicit Time Integration Scheme for Finite Volume Radiation-Hydrodynamics
- Non-LTE radiation hydrodynamics in PLUTO
- Time-dependent Multi-group Multidimensional Relativistic Radiative Transfer Code Based On Spherical Harmonic Discrete Ordinate Method
- A Spatial-Temporal asymptotic preserving scheme for radiation magnetohydrodynamics in the equilibrium and non-equilibrium diffusion limit
- A new ionisation network and radiation transport module in PLUTO
- Solving the Riemann Problem for Realistic Astrophysical Fluids
- On the application of Jacobian-free Riemann solvers for relativistic radiation magnetohydrodynamics under M1 closure
- Multidimensional half-moment multigroup radiative transfer. Improving moment-based thermal models of circumstellar disks
- Evolution of jets driven by relativistic radiation hydrodynamics as Long and Low Luminosity GRBs
- Effects of Opacity Temperature Dependence on Radiatively Accelerated Clouds
- The time step constraint in radiation hydrodynamics
- Future Simulations of Tidal Disruption Events
- Nonlinear Evolution of the Radiation-Driven Magneto-Acoustic Instability (RMI)
- Diffuse Radiation from the Aquila Rift
- Radiation-magnetohydrodynamics with MPI-AMRVAC using flux-limited diffusion
- Multigroup Radiation Diffusion on a Moving Mesh: Implementation in RICH and Application to Tidal Disruption Events
- Sub-photospheric fluctuations in magnetized radiative envelopes: contribution from unstable magnetosonic waves
- Numerical Methods for Simulating Star Formation
- Effects of Strong Photospheric Dissipation on the Spectra and Structure of Accretion Disks with Non-zero Inner Torque
- A radiation hydrodynamics scheme on adaptive meshes using the Variable Eddington Tensor (VET) closure