Multidimensional Boltzmann Neutrino Transport Code in Full General Relativity for Core-collapse Simulations
arXiv:2010.10780 · doi:10.3847/1538-4357/abe1bf
Abstract
We develop a neutrino transfer code for core-collapse simulations, that directly solves the multidimensional Boltzmann equations in full general relativity. We employ the discrete ordinate method, which discretizes the six dimensional phase space. The code is an extension of our special relativistic code coupled to a Newtonian hydrodynamics code, which is currently employed for core-collapse supernova simulations. In order to demonstrate our code's capability to treat general relativistic effects, we conduct some tests: we first compute the free streaming of neutrinos in the Schwarzschild and Kerr spacetimes and compare the results with the geodesic curves; in the Schwarzschild case we deploy not only a 1-dimensional grid in space under spherical symmetry but also a 2-dimensional spatial mesh under axisymmetry in order to assess the capability of the code to compute the spatial advection of neutrinos; secondly, we calculate the neutrino transport in a fixed matter background, which is taken from a core-collapse supernova simulation with our general relativistic but spherically symmetric Boltzmann-hydrodynamics code, to obtain a steady neutrino distribution; the results are compared with those given by the latter code.
arXiv comment23 pages, 19 figures, accepted version
References in corpus (48)
- On the Numerical Integration of Einstein's Field Equations
- Explosion Mechanisms of Core-Collapse Supernovae
- Relativistic Equation of State of Nuclear Matter for Supernova and Neutron Star
- Core-Collapse Supernova Explosion Theory
- Perspectives on Core-Collapse Supernova Theory
- Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport. I. Numerical method and results for a 15 M_sun star
- Probing the gravitational well: No supernova explosion in spherical symmetry with general relativistic Boltzmann neutrino transport
- The Overarching Framework of Core-Collapse Supernova Explosions as Revealed by 3D Fornax Simulations
- Postbounce evolution of core-collapse supernovae: Long-term effects of equation of state
- A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code for Core-Collapse Supernovae II. Relativistic Explosion Models of Core-Collapse Supernovae
- Truncated Moment Formalism for Radiation Hydrodynamics in Numerical Relativity
- The isotropic diffusion source approximation for supernova neutrino transport
- A new multi-dimensional general relativistic neutrino hydrodynamics code for core-collapse supernovae. I. Method and code tests in spherical symmetry
- General-Relativistic Simulations of Three-Dimensional Core-Collapse Supernovae
- A Successful 3D Core-Collapse Supernova Explosion Model
- Full Transport Model of GW170817-Like Disk Produces a Blue Kilonova
- The explosion mechanism of core-collapse supernovae: progress in supernova theory and experiments
- Global Comparison of Core-Collapse Supernova Simulations in Spherical Symmetry
- Three-Dimensional Supernova Explosion Simulations of 9-, 10-, 11-, 12-, and 13-M Stars
- General Relativistic Three-Dimensional Multi-Group Neutrino Radiation-Hydrodynamics Simulations of Core-Collapse Supernovae
- A New Gravitational-Wave Signature from Standing Accretion Shock Instabilities in Supernovae
- grmonty: a Monte Carlo Code for Relativistic Radiative Transport
- Neutrino Transfer in Three Dimensions for Core-Collapse Supernovae. I. Static Configurations
- Fully General Relativistic Simulations of Core-Collapse Supernovae with An Approximate Neutrino Transport
- Two Dimensional Core-Collapse Supernova Explosions Aided by General Relativity with Multidimensional Neutrino Transport
- Magnetorotational Explosion of A Massive Star Supported by Neutrino Heating in General Relativistic Three Dimensional Simulations
- A New Monte Carlo Method for Time-Dependent Neutrino Radiation Transport
- Three-dimensional Boltzmann-Hydro code for core-collapse in massive stars I. special relativistic treatments
- Simulations of core-collapse supernovae in spatial axisymmetry with full Boltzmann neutrino transport
- Numerical Relativity in Spherical Polar Coordinates: Evolution Calculations with the BSSN Formulation
- Core-collapse supernova simulations in one and two dimensions: comparison of codes and approximations
- A New Spherical Harmonics Scheme for Multi-Dimensional Radiation Transport I: Static Matter Configurations
- Monte-Carlo neutrino transport in neutron star merger simulations
- Should One Use the Ray-by-Ray Approximation in Core-Collapse Supernova Simulations?
- A Detailed Comparison of Multi-Dimensional Boltzmann Neutrino Transport Methods in Core-Collapse Supernovae
- A Monte Carlo Code for Relativistic Radiation Transport Around Kerr Black Holes
- Three-dimensional Boltzmann-Hydro code for core-collapse in massive stars II. The Implementation of moving-mesh for neutron star kicks
- Evaluating radiation transport errors in merger simulations using a Monte-Carlo algorithm
- A 3D Simulation of a Neutrino-Driven Supernova Explosion Aided By Convection and Magnetic Fields
- Core-collapse supernovae in the hall of mirrors. A three-dimensional code-comparison project
- On the Neutrino Distributions in Phase Space for the Rotating Core-collapse Supernova Simulated with a Boltzmann-neutrino-radiation-hydrodynamics Code
- : Radiation GRMHD for Neutrino-Driven Accretion Flows
- Simulations of the Early Post-Bounce Phase of Core-Collapse Supernovae in Three-Dimensional Space with Full Boltzmann Neutrino Transport
- Three-Dimensional Boltzmann-Hydro Code for core-collapse in massive stars III. A New method for momentum feedback from neutrino to matter
- The Impact of Different Neutrino Transport Methods on Multidimensional Core-collapse Supernova Simulations
- The Boltzmann-radiation-hydrodynamics Simulations of Core-collapse Supernovae with Different Equations of State: the Role of Nuclear Composition and the Behavior of Neutrinos
- A Novel Multi-Dimensional Boltzmann Neutrino Transport Scheme for Core-Collapse Supernovae
- General relativistic neutrino transport using spectral methods
Cited by in corpus (14)
- General-Relativistic Quantum-Kinetics Neutrino Transport
- Protoneutron Star Convection Simulated with a New General Relativistic Boltzmann Neutrino Radiation-Hydrodynamics Code
- Efficient estimation method for time evolution of proto-neutron star mass and radius from supernova neutrino signal
- Nuclei in Core-Collapse Supernovae Engine
- Gray Two-moment Neutrino Transport: Comprehensive Tests and Improvements for Supernova Simulations
- Leptonic and semi-leptonic neutrino interactions with muons in the proto-neutron star cooling
- Detectability of Late-time Supernova Neutrinos with Fallback Accretion onto Protoneutron star
- Comparative Testing of Subgrid Models for Fast Neutrino Flavor Conversions in Core-collapse Supernova Simulations
- Diagnosing electron-neutrino lepton number crossings in core-collapse supernovae: A comparison of methods
- 3D Photon Conserving Code for Time-dependent General Relativistic Radiative Transfer : CARTOON
- Electron-neutrino lepton number crossings: Variations with the supernova core physics
- A Relativistic Formula for the Multiple Scattering of Photons
- Asymmetric emissions of neutrinos in the cooling of rotating proto-neutron stars
- Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase