Elasticity suppresses the magnetorotational instability in neutron-star crusts unless the star spins faster than roughly 300 Hz, so pre-merger magnetic field amplification requires a rapidly rotating binary.
Premerger phenomena in neutron-star binary coalescences
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Renormalized dynamical tidal response functions for non-rotating black holes in GR carry inevitable ambiguities from renormalization scheme and flow initial condition, yielding scheme-dependent dynamical tidal Love numbers after MST-worldline EFT matching.
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Magnetorotational instabilities in solids: Application to neutron-star crusts
Elasticity suppresses the magnetorotational instability in neutron-star crusts unless the star spins faster than roughly 300 Hz, so pre-merger magnetic field amplification requires a rapidly rotating binary.
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Dynamical Tidal Response of Non-rotating Black Holes: Connecting the MST Formalism and Worldline EFT
Renormalized dynamical tidal response functions for non-rotating black holes in GR carry inevitable ambiguities from renormalization scheme and flow initial condition, yielding scheme-dependent dynamical tidal Love numbers after MST-worldline EFT matching.