Interlinking internal and external magnetic fields of relativistically rotating neutron stars
D. Ntotsikas, K.N. Gourgouliatos

TL;DR
This paper develops a comprehensive model linking internal and external magnetic fields of rotating neutron stars, revealing how internal twists influence magnetospheric structure and star spin-down, with implications for pulsar and magnetar behavior.
Contribution
It introduces a global solution connecting internal and external magnetic fields, highlighting the impact of internal twists and magnetospheric currents on neutron star dynamics and emissions.
Findings
Internal magnetic twist affects external field structure.
Magnetospheric currents influence internal field volume.
Transient behavior may result from magnetic field dissipation.
Abstract
This work presents a global solution for the internal and the external field of an axisymmetric rotating neutron star. It is shown that the twist of the internal field affects the external field, by increasing the number of open field lines and eventually the spin-down rate of the star. This effect is far more drastic if the toroidal field, and consequently the poloidal current flowing within the star, is allowed to populate the closed field lines of the magnetosphere, rather than if it remains confined in the star. We further remark that the internal field structure depends on the presence of a twisted magnetosphere: if the twist current is not allowed to flow in the magnetosphere it only occupied a narrow toroid at the interior of the star, whereas if the twist currents are allowed to flow in the magnetosphere the internal toroidal field may occupy a significant volume of the stellar…
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