Superfluid Spin-up: Three-dimensional Simulations of Post-glitch Dynamics in Neutron Star Cores

Neutron stars show a steady decrease in their rotational frequency, occasionally interrupted by sudden spin-up events called glitches. The dynamics of a neutron star after a glitch involve the transfer of angular momentum from the crust (where the glitch is presumed to originate) to the liquid core,...

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Bibliographic Details

Published in:	The Astrophysical Journal
Main Authors:	J. R. Fuentes, Vanessa Graber
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Hydrodynamical simulations Neutron stars Neutron star cores Rotation powered pulsars Stellar interiors
Online Access:	https://doi.org/10.3847/1538-4357/ad77d5