Gravitational waves from known pulsars : results from the initial detector era
Aasi, J. and Lockerbie, N. A. and Tokmakov, K. V., LIGO Scientific Collaboration, Virgo Collaboration (2014) Gravitational waves from known pulsars : results from the initial detector era. Astrophysical Journal, 785 (2). 119. ISSN 1538-4357 (https://doi.org/10.1088/0004-637x/785/2/119)
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Abstract
We present the results of searches for gravitational waves from a large selection of pulsars using data from the most recent science runs (S6, VSR2 and VSR4) of the initial generation of interferometric gravitational wave detectors LIGO (Laser Interferometric Gravitational-wave Observatory) and Virgo. We do not see evidence for gravitational wave emission from any of the targeted sources but produce upper limits on the emission amplitude. We highlight the results from seven young pulsars with large spin-down luminosities. We reach within a factor of five of the canonical spin-down limit for all seven of these, whilst for the Crab and Vela pulsars we further surpass their spin-down limits. We present new or updated limits for 172 other pulsars (including both young and millisecond pulsars). Now that the detectors are undergoing major upgrades, and, for completeness, we bring together all of the most up-to-date results from all pulsars searched for during the operations of the first-generation LIGO, Virgo and GEO600 detectors. This gives a total of 195 pulsars including the most recent results described in this paper.
ORCID iDs
Aasi, J., Lockerbie, N. A. ORCID: https://orcid.org/0000-0002-1678-3260 and Tokmakov, K. V. ORCID: https://orcid.org/0000-0002-2808-6593;-
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Item type: Article ID code: 50707 Dates: DateEvent2 April 2014PublishedNotes: J. Aasi et al. 2014 The Astrophysical Journal, 785:119. © 2014. The American Astronomical Society. Subjects: Science > Astronomy
Science > PhysicsDepartment: Faculty of Science > Physics Depositing user: Pure Administrator Date deposited: 09 Dec 2014 14:41 Last modified: 11 Nov 2024 10:53 URI: https://strathprints.strath.ac.uk/id/eprint/50707