Effects of Rotation on 3D Core-Collapse Supernova Models for Low-Mass Progenitors
astro-ph.HE, astro-ph.SR
Submitted: 2026-07-07
Updated: 2026-09-14
Comments: Submitted to Ap.J
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Impact of the equation of state on core collapse supernovae I: the low-$T/|W|$ instability
- The period clustering of magnetars and X-ray dim isolated neutron stars
- Radio Pulsars: The Neutron Star Population & Fundamental Physics
- A Three-Dimensional Exploration of Magnetic Fields, Rotation, and Shock Revival in a $39 M_\odot$ Core-Collapse Supernova Progenitor
- Gravitational Waves from Core-Collapse Supernovae
- Three-Dimensional Simulations of Neutrino-Driven Core-Collapse Supernovae from Low-Mass Single and Binary Star Progenitors
- 3D full-GR simulations of magnetorotational core-collapse supernovae on GPUs: A systematic study of rotation rates and magnetic fields
- Anisotropic emission of neutrino and gravitational-wave signals from rapidly rotating core-collapse supernovae
- Simulated 3D $^{56}$Ni Distributions of Type IIp Supernovae
- Neutrino-Driven Winds in Three-Dimensional Core-Collapse Supernova Simulations
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