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Induced Magnetic Field in Accretion Disks Around Neutron Stars: Discussion
by Magnetosphere: Maintaining Habitability on EarthMarch 8th, 2024
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This paper explores the interaction between accretion disks and neutron star magnetic fields, presenting a detailed model.
This paper is available on arxiv under CC 4.0 license.
Authors:
(1) A. V. Kuzin, Sternberg Astronomical Institute, Moscow, Russia and E-mail: alv.kuzin@gmail.com.
Table of Links
Model of Disk and Neutron Star
The Solution for the Induced Field
5. DISCUSSION
5.1. Axisymmetric component
5.2. Possible azimuthal-dependent contributions
It is unclear to what extent the φ-dependent components of the dipolar field penetrate the disk. In case they do not penetrate the disk at all, the induced field is given by b(r, z). Lai (1999) attempted to build a model of the induced field in this scenario (the ”Hybrid model”).
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