The Dzhanibekov Effect as a Possible Source of Magnetar Activity

Fuente: arXiv
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Main Authors: Wada, Tomoki, Shimoda, Jiro
Format: Preprint
Published: 2024
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author Wada, Tomoki
Shimoda, Jiro
author_facet Wada, Tomoki
Shimoda, Jiro
contents Magnetars, which are neutron stars with strong magnetic fields, exhibit occasional bursting activities. The shape of a magnetar is not perfectly spherical due to the Lorentz force exerted by its strong magnetic fields and is described as a triaxial body. We study the unstable free precession in a triaxial magnetar; one of the principal axes undergoes an upside-down flip. This flip is known as the Dzhanibekov effect. We find that during the flip, the Euler force can suddenly disturb the force balance on the surface layer of the magnetar, potentially leading to plastic flow of the layer. This, in turn, may trigger different forms of magnetar activity, such as the emission of the bursts and/or of gravitational waves.
format Preprint
id arxiv_https___arxiv_org_abs_2401_16783
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle The Dzhanibekov Effect as a Possible Source of Magnetar Activity
Wada, Tomoki
Shimoda, Jiro
High Energy Astrophysical Phenomena
Magnetars, which are neutron stars with strong magnetic fields, exhibit occasional bursting activities. The shape of a magnetar is not perfectly spherical due to the Lorentz force exerted by its strong magnetic fields and is described as a triaxial body. We study the unstable free precession in a triaxial magnetar; one of the principal axes undergoes an upside-down flip. This flip is known as the Dzhanibekov effect. We find that during the flip, the Euler force can suddenly disturb the force balance on the surface layer of the magnetar, potentially leading to plastic flow of the layer. This, in turn, may trigger different forms of magnetar activity, such as the emission of the bursts and/or of gravitational waves.
title The Dzhanibekov Effect as a Possible Source of Magnetar Activity
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2401.16783