A neutron star in a compact binary generates relativistic Alfven wings that carry most of the intersected electromagnetic power and may produce periodic pulsar-like emission.
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2026 2verdicts
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Plane-parallel analysis finds MRI operates in solids only when magnetic tension exceeds shear modulus, requiring spin frequencies ≳300 Hz for crust amplification in neutron-star mergers.
citing papers explorer
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Alfven-winged pulsar
A neutron star in a compact binary generates relativistic Alfven wings that carry most of the intersected electromagnetic power and may produce periodic pulsar-like emission.
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Magneto-rotational instabilities in solids: application to neutron-star crusts
Plane-parallel analysis finds MRI operates in solids only when magnetic tension exceeds shear modulus, requiring spin frequencies ≳300 Hz for crust amplification in neutron-star mergers.