Supernova Simulations

Understand

Magnetohydrodynamic simulations of core-collapse supernovae have become increasingly mature and important in recent years.

• Magnetic fields take center stage in scenarios for explaining hypernova explosions, but are now also considered in supernova theory more broadly as an important factor even in neutrino-driven explosions, especially in the context of neutron star birth properties.
• Here we present an overview of simulation approaches currently used for magnetohydrodynamic supernova simulations and sketch essential physical concepts for understanding the role of magnetic fields in supernovae of slowly or rapidly rotating massive stars.
• We review progress on simulations of neutrino-driven supernovae, magnetorotational supernovae, and the relevant field amplification processes.