Binary neutron star mergers: a review of Einstein's richest laboratory

L Baiotti, L Rezzolla - Reports on Progress in Physics, 2017 - iopscience.iop.org
In a single process, the merger of binary neutron star systems combines extreme gravity, the
copious emission of gravitational waves, complex microphysics and electromagnetic …

Physical, numerical, and computational challenges of modeling neutrino transport in core-collapse supernovae

A Mezzacappa, E Endeve, OEB Messer… - Living Reviews in …, 2020 - Springer
The proposal that core collapse supernovae are neutrino driven is still the subject of active
investigation more than 50 years after the seminal paper by Colgate and White. The modern …

MPI-AMRVAC 3.0: Updates to an open-source simulation framework

R Keppens, BP Braileanu, Y Zhou, W Ruan… - Astronomy & …, 2023 - aanda.org
Context. Computational astrophysics nowadays routinely combines grid-adaptive
capabilities with modern shock-capturing, high resolution spatio-temporal integration …

Spin-induced black hole spontaneous scalarization

A Dima, E Barausse, N Franchini, TP Sotiriou - Physical Review Letters, 2020 - APS
We study scalar fields in a black hole background and show that, when the scalar is suitably
coupled to curvature, rapid rotation can induce a tachyonic instability. This instability, which …

PETSc users manual

S Balay, S Abhyankar, M Adams, J Brown, P Brune… - 2019 - ora.ox.ac.uk
The Portable, Extensible Toolkit for Scientific Computation (PETSc), is a suite of data
structures and routines for the scalable (parallel) solution of scientific applications modeled …

Numerical methods for kinetic equations

G Dimarco, L Pareschi - Acta Numerica, 2014 - cambridge.org
In this survey we consider the development and mathematical analysis of numerical
methods for kinetic partial differential equations. Kinetic equations represent a way of …

The event horizon general relativistic magnetohydrodynamic code comparison project

O Porth, K Chatterjee, R Narayan… - The Astrophysical …, 2019 - iopscience.iop.org
Fully general relativistic models of astrophysical sources are in high demand, not only since
the discovery of gravitational waves emitted from merging stellar mass black holes (Abbott et …

Three-dimensional general relativistic radiation magnetohydrodynamical simulation of super-Eddington accretion, using a new code harmrad with M1 closure

JC McKinney, A Tchekhovskoy… - Monthly Notices of …, 2014 - academic.oup.com
Black hole (BH) accretion flows and jets are dynamic hot relativistic magnetized plasma
flows whose radiative opacity can significantly affect flow structure and behaviour. We …

PETSc/TS: A modern scalable ODE/DAE solver library

S Abhyankar, J Brown, EM Constantinescu… - arXiv preprint arXiv …, 2018 - arxiv.org
High-quality ordinary differential equation (ODE) solver libraries have a long history, going
back to the 1970s. Over the past several years we have implemented, on top of the PETSc …

Asymptotic-preserving schemes for multiscale physical problems

S Jin - Acta Numerica, 2022 - cambridge.org
We present the asymptotic transitions from microscopic to macroscopic physics, their
computational challenges and the asymptotic-preserving (AP) strategies to compute …