Twisted magnetic fields inside a neutron star alter its external magnetosphere and spin-down power, with the effect up to four times stronger when the twist current reaches the closed magnetospheric field lines.
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Interlinking internal and external magnetic fields of relativistically rotating neutron stars
Twisted magnetic fields inside a neutron star alter its external magnetosphere and spin-down power, with the effect up to four times stronger when the twist current reaches the closed magnetospheric field lines.