Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/7740
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dc.contributor.authorLIGO Scientific Collaboration; Virgo Collaboration; KAGRA Collaboration; Abbott, Ren_US
dc.contributor.authorSOURADEEP, TARUN et al.en_US
dc.date.accessioned2023-04-21T09:28:52Z
dc.date.available2023-04-21T09:28:52Z
dc.date.issued2022-11en_US
dc.identifier.citationPhysical Review D, 106(10), 102008.en_US
dc.identifier.issn2470-0010en_US
dc.identifier.issn2470-0029en_US
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.106.102008en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/7740
dc.description.abstractWe present results of an all-sky search for continuous gravitational waves which can be produced by spinning neutron stars with an asymmetry around their rotation axis, using data from the third observing run of the Advanced LIGO and Advanced Virgo detectors. Four different analysis methods are used to search in a gravitational-wave frequency band from 10 to 2048 Hz and a first frequency derivative from −10−8 to 10−9 Hz/s. No statistically significant periodic gravitational-wave signal is observed by any of the four searches. As a result, upper limits on the gravitational-wave strain amplitude h0 are calculated. The best upper limits are obtained in the frequency range of 100 to 200 Hz and they are ∼1.1×10−25 at 95% confidence level. The minimum upper limit of 1.10×10−25 is achieved at a frequency 111.5 Hz. We also place constraints on the rates and abundances of nearby planetary- and asteroid-mass primordial black holes that could give rise to continuous gravitational-wave signalsen_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectMountainsen_US
dc.subjectPulsarsen_US
dc.subject2022en_US
dc.titleAll-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 dataen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePhysical Review Den_US
dc.publication.originofpublisherForeignen_US
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