arXiv (All)
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Superradiant and dynamical spin-down of neutron stars with gravitational wave implications
general-relativity-and-quantum-cosmologyhigh-energy-astrophysical-phenomenasolar-and-stellar-astrophysics
Neutron stars such as pulsars and magnetars lose angular momentum primarily through electromagnetic dipole radiation, gravitational waves, $r$-mode oscillation. However, spin variations, particularly enhanced spin-down rates, indicate additional spin-down mechanisms. We propose superradiant spin-dow
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