Constraints on gravitational waves from the 2024 Vela pulsar glitch

Abac, A. G., Abouelfettouh, I., Acernese, F., Ackley, K., Adamcewicz, C., Al-Shammari, S., Amarasinghege, O., Bergamin, F., Divyajyoti, D. ORCID: https://orcid.org/0000-0002-2787-1012, Dooley, K. L. ORCID: https://orcid.org/0000-0002-1636-0233, Fairhurst, S. ORCID: https://orcid.org/0000-0001-8480-1961, Gottel, A. ORCID: https://orcid.org/0000-0002-6215-4641, Grote, H. ORCID: https://orcid.org/0000-0002-0797-3943, Hannam, M. D. ORCID: https://orcid.org/0000-0001-5571-325X, Higginbotham, S., Javed, W. ORCID: https://orcid.org/0009-0009-1471-7890, Kinnear, M., Kokeyama, K. ORCID: https://orcid.org/0000-0002-2896-1992, Kuntimaddi, N., MacLeod, D. M. ORCID: https://orcid.org/0000-0002-1395-8694, Norman, M., North, C., Patra, A., Patterson, B., Pearce, T., Raymond, V. ORCID: https://orcid.org/0000-0003-0066-0095, Schutz, B. F. ORCID: https://orcid.org/0000-0001-9487-6983, Skliris, V., Sutton, P. J. ORCID: https://orcid.org/0000-0003-1614-3922, Tanioka, S. and Tsang, T. 2026. Constraints on gravitational waves from the 2024 Vela pulsar glitch. The Astrophysical Journal 1005 (1) , 12. 10.3847/1538-4357/ae63bc

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Abstract

Among known neutron stars, the Vela pulsar is one of the best targets for gravitational-wave searches. It is also one of the most prolific in terms of glitches, which are sudden frequency changes in a pulsar’s rotation. Such glitches could cause a variety of transient gravitational-wave signals. Here, we search for signals associated with a Vela glitch on 2024 April 29 in data of the two LIGO detectors from the fourth LIGO–Virgo–KAGRA observing run. We search both for seconds-scale burst-like emission, primarily from fundamental (f-)mode oscillations, and for longer quasi-monochromatic transients up to 4 months in duration, primarily from quasi-static quadrupolar deformations. We find no significant detection candidates, but for the first time we set direct observational upper limits on gravitational strain amplitude that are stricter than what can be indirectly inferred from the overall glitch energy scale. We discuss the short- and long-duration observational constraints in the context of specific emission models. These results demonstrate the potential of gravitational-wave probes of glitching pulsars as detector sensitivity continues to improve.

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Schools > Physics and Astronomy
Additional Information:	For full author list see https://doi.org/10.3847/1538-4357/ae63bc License information from Publisher: LICENSE 1: URL: https://creativecommons.org/licenses/by/4.0/, Type: cc-by
Publisher:	American Astronomical Society
ISSN:	0004-637X
Date of First Compliant Deposit:	24 June 2026
Date of Acceptance:	4 April 2026
Last Modified:	07 Aug 2026 22:32
URI:	https://orca.cardiff.ac.uk/id/eprint/187728

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