scholarly journals Fermion zero-mode influence on neutron-star magnetic field evolution

2009 ◽  
Vol 397 (2) ◽  
pp. 1027-1031 ◽  
Author(s):  
P. B. Jones
Keyword(s):  
Magnetic Field ◽  
Neutron Star ◽  
Zero Mode ◽  
Field Evolution ◽  
Fermion Zero Mode

scholarly journals Magnetic Field Evolution in Neutron Star Crusts Due to the Hall Effect and Ohmic Decay

2004 ◽  
Vol 609 (2) ◽  
pp. 999-1017 ◽  
Author(s):  
Andrew Cumming ◽  
Phil Arras ◽  
Ellen Zweibel
Keyword(s):  
Magnetic Field ◽  
Neutron Star ◽  
Hall Effect ◽  
Field Evolution

Neutron Star Magnetic Field Evolution, Crust Movement, and Glitches

1998 ◽  
Vol 492 (1) ◽  
pp. 267-280 ◽  
Author(s):  
Malvin Ruderman ◽  
Tianhua Zhu ◽  
Kaiyou Chen
Keyword(s):  
Magnetic Field ◽  
Neutron Star ◽  
Field Evolution

scholarly journals On the magnetic field evolution time-scale in superconducting neutron star cores

2017 ◽  
Vol 469 (4) ◽  
pp. 4979-4984 ◽  
Author(s):  
Andrea Passamonti ◽  
Taner Akgün ◽  
José A. Pons ◽  
Juan A. Miralles
Keyword(s):  
Magnetic Field ◽  
Neutron Star ◽  
Time Scale ◽  
Evolution Time ◽  
Field Evolution ◽  
The Magnetic Field

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

2020 ◽  
Vol 494 (3) ◽  
pp. 3790-3798 ◽  
Author(s):  
Yasufumi Kojima ◽  
Kazuki Suzuki
Keyword(s):  
Magnetic Field ◽  
Neutron Star ◽  
Lorentz Force ◽  
Large Scale ◽  
Magnetic Energy ◽  
Fluid Motion ◽  
Navier Stokes Equation ◽  
Ohmic Dissipation ◽  
Neutron Star Crust ◽  
Field Evolution

ABSTRACT 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.

scholarly journals Erratum: “Neutron Star Magnetic Field Evolution, Crust Movement, and Glitches” (ApJ, 492, 267 [1998])

1998 ◽  
Vol 502 (2) ◽  
pp. 1027-1027 ◽  
Author(s):  
Malvin Ruderman ◽  
Tianhua Zhu ◽  
Kaiyou Chen
Keyword(s):  
Magnetic Field ◽  
Neutron Star ◽  
Field Evolution

Magnetic Field Evolution in Merging Clusters of Galaxies

1999 ◽  
Vol 518 (2) ◽  
pp. 594-602 ◽  
Author(s):  
Kurt Roettiger ◽  
James M. Stone ◽  
Jack O. Burns
Keyword(s):  
Magnetic Field ◽  
Clusters Of Galaxies ◽  
Field Evolution
Sign in / Sign up

Export Citation Format

Share Document