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Induced Magnetic Field in Accretion Disks Around Neutron Stars: Discussionby@magnetosphere
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Induced Magnetic Field in Accretion Disks Around Neutron Stars: Discussion

by Magnetosphere: Maintaining Habitability on Earth
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March 8th, 2024
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This paper explores the interaction between accretion disks and neutron star magnetic fields, presenting a detailed model.
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Magnetosphere: Maintaining Habitability on Earth

Magnetosphere: Maintaining Habitability on Earth

@magnetosphere

Shielding the planet from harmful solar radiation.

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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.

Abstract and Introduction

Model of Disk and Neutron Star

Main Equations

The Solution for the Induced Field

Discussion

Conclusion and References

5. DISCUSSION

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5.1. Axisymmetric component


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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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