Induced Magnetic Field in Accretion Disks Around Neutron Stars: Discussion

Written by @magnetosphere | Published on 2024/3/8

TL;DR —

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

Abstract and Introduction

Model of Disk and Neutron Star

Main Equations

The Solution for the Induced Field

Discussion

Conclusion and References

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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