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Searches for Continuous-Wave Gravitational Radiation

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arxiv 2206.06447 v2 pith:ZQ6RGFPL submitted 2022-06-13 astro-ph.HE gr-qc

Keith Riles This is my paper · ORCID
classification astro-ph.HEgr-qc
keywords gravitationalcontinuous-wavediscoverypotentialprospectssourceswavebecome
verification ladder T0 review T1 audit T2 compute T3 formal
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Now that detection of gravitational wave signals from the coalescence of extra-galactic compact binary star mergers has become nearly routine, it is intriguing to consider other potential gravitational wave signatures. Here we examine the prospects for discovery of continuous gravitational waves from fast-spinning neutron stars in our own galaxy and from more exotic sources. Potential continuous-wave sources are reviewed, search methodologies and results presented and prospects for imminent discovery discussed.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Search for continuous gravitational waves from the pulsar J0435+3233

    gr-qc 2026-07 accept novelty 6.0 of 10

    A LIGO O4a search for continuous gravitational waves from millisecond pulsar J0435+3233 finds no signal, setting h0<5.8×10^-27 at 95% confidence and an ellipticity limit of 1.6×10^-8.

  2. Directional Search for Persistent Gravitational Waves: Results from the First Part of LIGO-Virgo-KAGRA's Fourth Observing Run

    gr-qc 2025-10 conditional novelty 6.0 of 10

    An 8.3-year LIGO–Virgo–KAGRA search for persistent, direction-dependent gravitational waves finds no signal and yields the most restrictive upper limits to date on anisotropic backgrounds and targeted sources.

  3. Guiding interferometer improvements with the frequency-dependent inspiral range

    astro-ph.IM 2025-02 conditional novelty 6.0 of 10

    The cumulative normalized range and its two-curve difference make it easier to see which frequency bands actually limit a gravitational-wave detector's inspiral range.

  4. Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO

    astro-ph.HE 2026-07 accept novelty 3.5 of 10

    SKAO's sensitivity, surveys and sub-arraying will deliver tighter NS mass, MoI, spin, glitch and precession constraints that, with X-ray and GW data, probe cold ultra-dense matter.

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