In 3D GRMHD simulations, neutron star rotation delays Tayler, kink, and Parker instabilities, so faster-spinning models retain more magnetic energy over 10 Alfven times.
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Impact of rotation on magnetic field stability and orientation in isolated neutron stars
In 3D GRMHD simulations, neutron star rotation delays Tayler, kink, and Parker instabilities, so faster-spinning models retain more magnetic energy over 10 Alfven times.