The authors implement and validate nuclear networks coupled to GRRMHD with M1 neutrino transport in Gmunu, showing effects on core-collapse supernova shock revival and composition.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Nine axisymmetric GR neutrino MHD simulations of AIC produce proto-magnetars (1.15-1.45 Msun, 2.9-4.9 kHz) that exhibit universal magnetic energy evolution and episodic instabilities when magnetic energy exceeds rotational energy.
citing papers explorer
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Toward First-Principles Multi-Messenger Predictions: Coupling Nuclear Networks with GR Radiation-MHD in {\tt Gmunu}
The authors implement and validate nuclear networks coupled to GRRMHD with M1 neutrino transport in Gmunu, showing effects on core-collapse supernova shock revival and composition.
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Magnetar Formation from Accretion Induced Collapse of White Dwarfs
Nine axisymmetric GR neutrino MHD simulations of AIC produce proto-magnetars (1.15-1.45 Msun, 2.9-4.9 kHz) that exhibit universal magnetic energy evolution and episodic instabilities when magnetic energy exceeds rotational energy.