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Probing the interior of neutron stars with gravitational waves

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arxiv astro-ph/0506681 v1 pith:SYXH4CWZ submitted 2005-06-28 astro-ph

L.K. Tsui , P.T. Leung This is my paper · ORCID
classification astro-ph
keywords gravitationalneutronaccurateadditionapplydampingdensitydetermine
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abstract

We show here how the internal structure of a neutron star can be inferred from its gravitational wave spectrum. Under the premise that the frequencies and damping rates of a few $w$-mode oscillations are found, we apply an inversion scheme to determine its mass, radius and density distribution. In addition, accurate equation of state of nuclear matter can also be determined.

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  1. Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors

    astro-ph.HE 2025-02 conditional novelty 5.0 of 10

    Future gravitational wave detectors should measure most neutron star radii to within about 5%, while current detectors give biased and imprecise estimates.

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