activity
20242026
collaborators

12 papers

astro-ph.HE2026

Magnetic field dynamics in isolated neutron stars with an external dipole field

Aurora Capobianco, William Cook, Sebastiano Bernuzzi +2

Neutron stars can harbor extremely strong magnetic fields, yet the structure and stability of their magnetic field configuration remain poorly understood. Observations of pulsars i…

astro-ph.HE2026

Subgrid Modelling for Relativistic Magnetohydrodynamics with Machine Learning

William Cook, Sebastiano Bernuzzi

Resolving the impact of magnetic field instabilities in triggering small scale turbulent flow and the associated rearrangement of the field is of critical importance in understandi…

astro-ph.HE2026

Turbulence in Magnetised Neutron Stars

William Cook, Raj Kishor Joshi, Sebastiano Bernuzzi +2

The magnetic field configuration in the interior of neutron stars and its stability are open problems and may be impacted by the influence of a turbulent cascade within the star. A…

gr-qc2026

GR-Athena++: Binary Neutron Star Merger Simulations with Neutrino Transport

Boris Daszuta, Sebastiano Bernuzzi, Maximilian Jacobi +4

We present general-relativistic radiation magnetohydrodynamics simulations of binary neutron star mergers performed with GR-Athena++. Neutrino transport is treated using a moment-b…

astro-ph.HE2025

Magnetic Field Configurations in Binary Neutron Star Mergers I: Post-merger Remnant and Disk

Eduardo M. Gutiérrez, William Cook, David Radice +6

We present a suite of general relativistic magnetohydrodynamic (GRMHD) simulations of binary neutron star (BNS) mergers performed with the code GR-Athena++. We investigate how a di…

astro-ph.HE2025

Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta

William Cook, Eduardo M. Gutiérrez, Sebastiano Bernuzzi +6

We perform a series of simulations of magnetised Binary Neutron Star mergers, with varying magnetic field topologies in the initial data, as well as varying Equations of State, and…