CoCoNuT Meeting 2026

3D magnetorotational core-collapse supernova simulations with CoCoNuT

Not scheduled

20m

Building 56 (University of Southampton)

CoCoNuT meeting (9-11 Sept)

Speaker

Jade Powell (Swinburne University of Technology)

Description

We perform 3D simulations of supernovae with a variety of magnetic field strengths and rotation rates with the magnetohydrodynamical version of the CoCoNuT code. We simulate a 39 solar mass progenitor star with rapid rotation and three different magnetic field strengths, and a 15 solar mass progenitor with different equations of state, rotation rates, and weak magnetic fields. We discuss the impacts of the magnetic fields on the explosion dynamics, jets, compact remnant properties and gravitational-wave emission.