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.
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Free neutrons survive r-process freeze-out in fast ejecta of neutron star mergers and their beta-decay heating produces a visible early kilonova precursor for mass fractions above ~0.05.
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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.
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Nucleosynthesis in the fast ejecta of a neutron star merger
Free neutrons survive r-process freeze-out in fast ejecta of neutron star mergers and their beta-decay heating produces a visible early kilonova precursor for mass fractions above ~0.05.