RADAMESH: Cosmological Radiative Transfer for Adaptive Mesh Refinement Simulations
arXiv:1009.1625 · doi:10.1111/j.1365-2966.2010.17799.x
Abstract
We present a new three-dimensional radiative transfer (RT) code, RADAMESH, based on a ray-tracing, photon-conserving and adaptive (in space and time) scheme. RADAMESH uses a novel Monte Carlo approach to sample the radiation field within the computational domain on a "cell-by-cell" basis. Thanks to this algorithm, the computational efforts are now focused where actually needed, i.e. within the Ionization-fronts (I-fronts). This results in an increased accuracy level and, at the same time, a huge gain in computational speed with respect to a "classical" Monte Carlo RT, especially when combined with an Adaptive Mesh Refinement (AMR) scheme. Among several new features, RADAMESH is able to adaptively refine the computational mesh in correspondence of the I-fronts, allowing to fully resolve them within large, cosmological boxes. We follow the propagation of ionizing radiation from an arbitrary number of sources and from the recombination radiation produced by H and He. The chemical state of six species (HI, HII, HeI, HeII, HeIII, e) and gas temperatures are computed with a time-dependent, non-equilibrium chemistry solver. We present several validating tests of the code, including the standard tests from the RT Code Comparison Project and a new set of tests aimed at substantiating the new characteristics of RADAMESH. Using our AMR scheme, we show that properly resolving the I-front of a bright quasar during Reionization produces a large increase of the predicted gas temperature within the whole HII region. Also, we discuss how H and He recombination radiation is able to substantially change the ionization state of both species (for the classical Stroemgren sphere test) with respect to the widely used "on-the-spot" approximation.
19 pages, 24 figures; accepted for publication in MNRAS, version with high-resolution figures is avalaible at http://www.ast.cam.ac.uk/~cantal/Papers/CP10.pdf
References in corpus (13)
- Radiative transfer simulations of cosmic reionization I: methodology and initial results
- Cosmological Radiative Transfer Codes Comparison Project I: The Static Density Field Tests
- A radiative transfer scheme for cosmological reionization based on a local Eddington tensor
- TRAPHIC - Radiative Transfer for Smoothed Particle Hydrodynamics Simulations
- An implementation of radiative transfer in the cosmological simulation code GADGET
- Lyman-alpha radiative transfer during the Epoch of Reionization: contribution to 21-cm signal fluctuations
- Mapping Neutral Hydrogen During Reionization with the Ly-alpha Emission from Quasar Ionization Fronts
- SPHRAY: A Smoothed Particle Hydrodynamics Ray Tracer for Radiative Transfer
- Theoretical calculations of the HI, HeI and HeII free-bound continuou emission spectra
- A New Moment Method for Continuum Radiative Transfer in Cosmological Reionization
- Block Structured Adaptive Mesh and Time Refinement for Hybrid, Hyperbolic + N-body Systems
- The Diffuse Nature of Stromgren Spheres
- Transport on Adaptive Random Lattices
Cited by in corpus (36)
- A model for cosmological simulations of galaxy formation physics
- A cosmic web filament revealed in Lyman-alpha emission around a luminous high-redshift quasar
- RAMSES-RT: Radiation hydrodynamics in the cosmological context
- Absorption line systems in simulated galaxies fed by cold streams
- The First Billion Years Project: The escape fraction of ionizing photons in the epoch of reionization
- Moving mesh cosmology: numerical techniques and global statistics
- Quasars Probing Quasars VI. Excess HI Absorption Within One Proper Mpc of z~2 Quasars
- Detection of dark galaxies and circum-galactic filaments fluorescently illuminated by a quasar at z=2.4
- Constraints on X-ray Emissions from the Reionization Era
- The large and small scale properties of the intergalactic gas in the Slug Ly-alpha nebula revealed by MUSE HeII emission observations
- The imprint of inhomogeneous HeII reionization on the HI and HeII Ly-alpha forest
- Confronting Simulations of Optically Thick Gas in Massive Halos with Observations at z=2-3
- The Stacked Lyman-Alpha Emission Profile from the Circum-Galactic Medium of z~2 Quasars
- Multi-frequency, thermally coupled radiative transfer with TRAPHIC: Method and tests
- The effect of intergalactic helium on hydrogen reionisation: implications for the sources of ionising photons at z > 6
- Quasar Ionization Front Lyα Emission in an Inhomogeneous Intergalactic Medium
- Probing the end of reionization with the near-zones of z > 6 QSOs
- Synthetic observations of star formation and the interstellar medium
- Optimized Multi-Frequency Spectra for Applications in Radiative Feedback and Cosmological Reionization
- AGN-driven helium reionization and the incidence of extended HeIII regions at redshift z>3
- Radiative transfer of energetic photons: X-rays and helium ionization in C2-Ray
- Baryon history and cosmic star formation in non-Gaussian cosmological models: numerical simulations
- A novel approach for accurate radiative transfer in cosmological hydrodynamic simulations
- Dynamics of H II regions around exiled O stars
- The Goldilocks problem of the quasar contribution to reionization
- Accuracy and Efficiency of Raytracing Photoionisation Algorithms
- Quasars as probes of cosmological reionization
- Radiation in equilibrium with plasma and plasma effects on cosmic microwave background
- Smoothed Particle Radiation Hydrodynamics: Two-Moment method with Local Eddington Tensor Closure
- The effect of recombination radiation on the temperature and ionization state of partially ionized gas
- A fast tree-based method for estimating column densities in Adaptive Mesh Refinement codes Influence of UV radiation field on the structure of molecular clouds
- Efficient Photo-heating Algorithms in Time-dependent Photo-ionization Simulations
- A comparison of numerical methods for computing the reionization of intergalacitc hydrogen and helium by a central radiating source
- Measuring photo-ionization rate and mean free path of HeII ionizing photons at : Evidence for late and rapid HeII reionization Part-II
- Rabacus: A Python Package for Analytic Cosmological Radiative Transfer Calculations
- Detecting the signature of helium reionization through 3HeII 3.46cm line-intensity mapping