SIMBAD references

2020MNRAS.494.3790K - Mon. Not. R. Astron. Soc., 494, 3790-3798 (2020)

Magnetic-field evolution with large-scale velocity circulation in a neutron-star crust.

KOJIMA Y. and SUZUKI K.

Abstract (from CDS):

We examine the effects of plastic flow that appear in a neutron-star crust when a magnetic stress exceeds the threshold. The dynamics involved are described using the Navier-Stokes equation comprising the viscous-flow term, and the velocity fields for the global circulation are determined using quasi-stationary approximation. We simulate the magnetic-field evolution by taking into consideration the Hall drift, Ohmic dissipation, and fluid motion induced by the Lorentz force. The decrease in the magnetic energy is enhanced, as the energy converts to the bulk motion energy and heat. It is found that the bulk velocity induced by the Lorentz force has a significant influence in the low-viscosity and strong-magnetic-field regimes. This effect is crucial near magnetar surfaces.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): stars: magnetars - stars: magnetic field - stars: neutron

Simbad objects: 9

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2020MNRAS.494.3790K and select 'bookmark this link' or equivalent in the popup menu


2021.03.04-13:58:11

© Université de Strasbourg/CNRS

    • Contact