Narrowband searches for continuous and long-duration transient gravitational waves from known pulsars in the LIGO-Virgo third observing run
Abbott, R. and Angelova, S. V. and Ben Yaala, M. and Gier, C. and Hill, P. and Reid, S. and Talbot, C. J. and Wallace, G. S., LIGO Scientific Collaboration (2022) Narrowband searches for continuous and long-duration transient gravitational waves from known pulsars in the LIGO-Virgo third observing run. The Astrophysical Journal, 932 (2). 133. ISSN 1538-4357 (https://doi.org/10.3847/1538-4357/ac6ad0)
Preview |
Text.
Filename: Abbott_etal_AJ_2022_Narrowband_searches_for_continuous_and_long_duration_transient_gravitational_waves_from_known_pulsars.pdf
Final Published Version License: Download (11MB)| Preview |
Abstract
Isolated neutron stars that are asymmetric with respect to their spin axis are possible sources of detectable continuous gravitational waves. This paper presents a fully coherent search for such signals from eighteen pulsars in data from LIGO and Virgo’s third observing run (O3). For known pulsars, efficient and sensitive matched-filter searches can be carried out if one assumes the gravitational radiation is phase-locked to the electromagnetic emission. In the search presented here, we relax this assumption and allow both the frequency and the time derivative of the frequency of the gravitational waves to vary in a small range around those inferred from electromagnetic observations. We find no evidence for continuous gravitational waves, and set upper limits on the strain amplitude for each target. These limits are more constraining for seven of the targets than the spin-down limit defined by ascribing all rotational energy loss to gravitational radiation. In an additional search, we look in O3 data for long-duration (hours–months) transient gravitational waves in the aftermath of pulsar glitches for six targets with a total of nine glitches. We report two marginal outliers from this search, but find no clear evidence for such emission either. The resulting duration-dependent strain upper limits do not surpass indirect energy constraints for any of these targets.
ORCID iDs
Abbott, R., Angelova, S. V., Ben Yaala, M. ORCID: https://orcid.org/0000-0002-6754-0875, Gier, C., Hill, P. ORCID: https://orcid.org/0000-0003-4826-3531, Reid, S., Talbot, C. J. and Wallace, G. S.;-
-
Item type: Article ID code: 81290 Dates: DateEvent27 June 2022Published21 March 2022AcceptedSubjects: Science > Physics > Optics. Light
Science > PhysicsDepartment: Faculty of Engineering > Biomedical Engineering Depositing user: Pure Administrator Date deposited: 28 Jun 2022 14:48 Last modified: 11 Nov 2024 13:32 URI: https://strathprints.strath.ac.uk/id/eprint/81290