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3D Simulations of Magnetoconvection in a Rapidly Rotating Supernova Progenitor (2023)
Journal Article
Varma, V., & Müller, B. (2023). 3D Simulations of Magnetoconvection in a Rapidly Rotating Supernova Progenitor. Monthly Notices of the Royal Astronomical Society, 526(4), 5249–5262. https://doi.org/10.1093/mnras/stad3113

We present a first 3D magnetohydrodynamic (MHD) simulation of oxygen, neon and carbon shell burning in a rapidly rotating 16M⊙ core-collapse supernova progenitor. We also run a purely hydrodynamic simulation for comparison. After $\mathord \approx 18... Read More about 3D Simulations of Magnetoconvection in a Rapidly Rotating Supernova Progenitor.

3D simulations of strongly magnetized non-rotating supernovae: explosion dynamics and remnant properties (2022)
Journal Article
Varma, V., Müller, B., & Schneider, F. R. N. (2022). 3D simulations of strongly magnetized non-rotating supernovae: explosion dynamics and remnant properties. Monthly Notices of the Royal Astronomical Society, 518(3), 3622-3636. https://doi.org/10.1093/mnras/stac3247

We investigate the impact of strong initial magnetic fields in core-collapse supernovae of non-rotating progenitors by simulating the collapse and explosion of a 16.9 M-circle dot star for a strong- and weak-field case assuming a twisted-torus field... Read More about 3D simulations of strongly magnetized non-rotating supernovae: explosion dynamics and remnant properties.