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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Model atmosphere fitting of 25,642 cool white dwarfs in DESI DR1 finds no photometric-spectroscopic mass discrepancy for DAs, magnetic DAs at all temperatures, increasing H/He ratios in He-atmosphere stars below ~10,000 K, and a rising He-atmosphere fraction due to convective mixing.
citing papers explorer
-
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.
-
A Detailed Model Atmosphere Analysis of Cool White Dwarfs in DESI DR1
Model atmosphere fitting of 25,642 cool white dwarfs in DESI DR1 finds no photometric-spectroscopic mass discrepancy for DAs, magnetic DAs at all temperatures, increasing H/He ratios in He-atmosphere stars below ~10,000 K, and a rising He-atmosphere fraction due to convective mixing.