A triple-star channel with two common envelope evolution phases produces merging black hole binaries with positive average χ_eff and a tail of negative values.
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3 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.
Hydrodynamic simulations of three pairs of jittering jets in a CCSN reproduce the ring-and-bar morphology of SNR G11.2-0.3.
citing papers explorer
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Stellar black hole binaries from two common envelope evolution phases in triple stellar systems
A triple-star channel with two common envelope evolution phases produces merging black hole binaries with positive average χ_eff and a tail of negative values.
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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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Reproducing morphological features in the supernova remnant G11.2-0.3 by simulating jittering jets
Hydrodynamic simulations of three pairs of jittering jets in a CCSN reproduce the ring-and-bar morphology of SNR G11.2-0.3.