Estimation of Electrical Conductivity and Magnetization Parameter of Neutron Star Crusts and Applied to the High-Braking-Index Pulsar PSR J1640-4631

Estimation of Electrical Conductivity and Magnetization Parameter of Neutron Star Crusts and Applied to the High-Braking-Index Pulsar PSR J1640-4631

Young pulsars are thought to be highly magnetized neutron stars (NSs). The crustal magnetic field of a NS usually decays at different timescales in the forms of Hall drift and Ohmic dissipation. The magnetization parameter <inline-formula> <math display="inline"> <semantics&...

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Bibliographic Details
Main Authors: Hui Wang, Zhi-Fu Gao, Huan-Yu Jia, Na Wang, Xiang-Dong Li
Format: Article
Language:English
Published: MDPI AG 2020-05-01
Series:Universe
Subjects:
neutron stars
conductivity
magnetization parameters
ohmic dissipation
hall drift
Online Access:https://www.mdpi.com/2218-1997/6/5/63

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https://www.mdpi.com/2218-1997/6/5/63

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