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The r-mode instability in rotating neutron stars

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arxiv gr-qc/0010102 v1 pith:K2GSOY7G submitted 2000-10-27 gr-qc astro-ph

N. Andersson , K.D. Kokkotas This is my paper
classification gr-qcastro-ph
keywords neutronstarsinstabilitydiscussr-moder-modesrotatingaccreting
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In this review we summarize the current understanding of the gravitational-wave driven instability associated with the so-called r-modes in rotating neutron stars. We discuss the nature of the r-modes, the detailed mechanics of the instability and its potential astrophysical significance. In particular we discuss results regarding the spin-evolution of nascent neutron stars, the detectability of r-mode gravitational waves and mechanisms limiting the spin-rate of accreting neutron stars in binary systems.

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Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 413 citations worldwide. Full citation record

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    Using causal BDNK hydrodynamics, the authors derive coupled gravitational-wave and viscous-mode equations for slowly rotating stars and find superradiant amplification at low frequencies.

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  3. Multi-wavelength Constraints on the Transient EP250905a

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  4. Hybrid Stars with Post-Merger Rotation Profiles

    gr-qc 2026-06 unverdicted novelty 5.0 of 10

    Differential rotation in hybrid stars with deconfinement phase transition allows quasi-toroidal configurations with quark matter rings and leads to degeneracies in rotational profiles at mass-radius curve intersections.

  5. Inferring neutron star properties through gravitational waves from r-modes and their relativistic counterparts

    astro-ph.HE 2024-06 unverdicted novelty 4.0 of 10

    Two inference frameworks are developed for neutron star properties from r-mode gravitational waves, one assuming electromagnetic distance and the other estimating distance via universal relations plus an assumed equat...

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