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Gravitational Waves and the Maximum Spin Frequency of Neutron Stars

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arxiv 1109.0536 v1 pith:XAXCKYLK submitted 2011-09-02 astro-ph.HE

Alessandro Patruno , Brynmor Haskell , Caroline D'Angelo (API , University of Amsterdam) This is my paper · ORCID
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keywords neutronx-rayexplaingravitationalmaximummillisecondpulsarsspin
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In this Letter we re-examine the idea that gravitational waves are required as a braking mechanism to explain the observed maximum spin-frequency of neutron stars. We show that for millisecond X-ray pulsars, the existence of spin equilibrium as set by the disk/magnetosphere interaction is sufficient to explain the observations. We show as well that no clear correlation exists between the neutron star magnetic field B and the X-ray outburst luminosity Lx when considering an enlarged sample size of millisecond X-ray pulsars.

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  1. Particle Probes with Superradiant Pulsars

    hep-ph 2019-08 conditional novelty 6.0 of 10

    The existence of PSR J1748-2446ad and PSR B1937+21 excludes ultralight scalars coupled to neutrons with masses near 10^-11 eV at couplings as small as 10^-6 times gravity.

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