A Multidimensional General-Relativistic Boltzmann Solver for Neutrino Transport: Implementation, Discretization and Optimization
astro-ph.HE, gr-qc, hep-ph
Submitted: 2026-09-25
Updated: 2026-09-25
Terminology
Sources
- Hydrodynamics of core-collapse supernovae and their progenitors
- Physical, numerical, and computational challenges of modeling neutrino transport in core-collapse supernovae
- Core-Collapse Supernova Explosion Theory
- Neutrinos from core-collapse supernovae
- Properties of Neutrino-driven Ejecta from the Remnant of Binary Neutron Star Merger : Purely Radiation Hydrodynamics Case
- Accurate muonic interactions in neutron star mergers and impact on heavy-element nucleosynthesis
- Neutrino transport in general relativistic neutron star merger simulations
- Dynamical Mass Ejection from Binary Neutron Star Mergers
- An Open-Source Neutrino Radiation Hydrodynamics Code for Core-Collapse Supernovae
- Fornax: a Flexible Code for Multiphysics Astrophysical Simulations
- M1 neutrino transport within the numerical-relativistic code BAM with application to low mass binary neutron star mergers
- ANRe-M1: a GPU-accelerated numerical relativity code with multi-energy M1 neutrino transport
- Neutrino transport in type II supernovae: Boltzmann solver vs. Monte Carlo method
- 2D Multi-Angle, Multi-Group Neutrino Radiation-Hydrodynamic Simulations of Postbounce Supernova Cores
- General relativistic neutrino transport using spectral methods
- Momentum Space Resolution Dependence in Boltzmann Neutrino Radiation Hydrodynamics Simulations of Core-collapse Supernovae
- A radiation-hydrodynamics scheme valid from the transport to the diffusion limit
- 3+1 Formalism and Bases of Numerical Relativity
- Solving the 3+1 GRMHD equations in the eXtended Conformally Flat Condition: the XNS code for magnetized neutron stars
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