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astro-ph.SR2026
Angular momentum transport in the convection zone of a 3D MHD simulation of a rapidly rotating core-collapse progenitor
Ryota Shimada, Lucy O. McNeill, Vishnu Varma +3
Rotation and magnetic fields in the cores of evolved massive stars in their final phase are thought to play an important role in the subsequent supernova explosion and the formatio…
astro-ph.HE2026
Resolution Dependence in Magnetohydrodynamic Simulations of Neutrino-Driven Core-Collapse Supernovae
Vishnu Varma, Bernhard Müller
We investigate the role of resolution and initial magnetic field strength on core-collapse supernovae in simulations of a non-rotating progenitor. Specificall…