Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/56451
Citations
Scopus Web of Science® Altmetric
?
?
Full metadata record
DC FieldValueLanguage
dc.contributor.authorAbbott, B.en
dc.contributor.authorAbbott, R.en
dc.contributor.authorAdhikari, R.en
dc.contributor.authorAjith, P.en
dc.contributor.authorAllen, B.en
dc.contributor.authorAllen, G.en
dc.contributor.authorAmin, R.en
dc.contributor.authorAnderson, D.en
dc.contributor.authorAnderson, S.en
dc.contributor.authorAnderson, W.en
dc.contributor.authorArain, M.en
dc.contributor.authorAraya, M.en
dc.contributor.authorArmandula, H.en
dc.contributor.authorArmor, P.en
dc.contributor.authorAso, Y.en
dc.contributor.authorAston, S.en
dc.contributor.authorAufmuth, P.en
dc.contributor.authorAulbert, C.en
dc.contributor.authorBabak, S.en
dc.contributor.authorBallmer, S.en
dc.contributor.authoret al.en
dc.date.issued2009en
dc.identifier.citationPhysical Review. D. Particles, Fields, Gravitation and Cosmology, 2009; 79(2):022001-1-022001-29en
dc.identifier.issn1550-7998en
dc.identifier.issn1550-2368en
dc.identifier.urihttp://hdl.handle.net/2440/56451-
dc.description.abstractA search for periodic gravitational waves, from sources such as isolated rapidly spinning neutron stars, was carried out using 510 h of data from the fourth LIGO science run (S4). The search was for quasimonochromatic waves in the frequency range from 50 to 1500 Hz, with a linear frequency drift f˙ (measured at the solar system barycenter) in the range -f/τ<f˙<0.1f/τ, where the minimum spin-down age τ was 1000 yr for signals below 300 Hz and 10 000 yr above 300 Hz. The main computational work of the search was distributed over approximately 100 000 computers volunteered by the general public. This large computing power allowed the use of a relatively long coherent integration time of 30 h, despite the large parameter space searched. No statistically significant signals were found. The sensitivity of the search is estimated, along with the fraction of parameter space that was vetoed because of contamination by instrumental artifacts. In the 100 to 200 Hz band, more than 90% of sources with dimensionless gravitational-wave strain amplitude greater than 10-23 would have been detected.en
dc.description.statementofresponsibilityB. Abbott... D. J. Hosken... J. Munch... P. J. Veitch...et al. (LIGO Scientific Collaboration)en
dc.language.isoenen
dc.publisherAmerican Physical Socen
dc.rights© 2009 The American Physical Societyen
dc.titleEinstein@Home search for periodic gravitational waves in LIGO S4 dataen
dc.typeJournal articleen
dc.identifier.rmid0020090128en
dc.identifier.doi10.1103/PhysRevD.79.022001en
dc.identifier.pubid39344-
pubs.library.collectionChemistry and Physics publicationsen
pubs.verification-statusVerifieden
pubs.publication-statusPublisheden
dc.identifier.orcidOttaway, D. [0000-0001-6794-1591]en
dc.identifier.orcidVeitch, P. [0000-0002-2597-435X]en
Appears in Collections:Chemistry and Physics publications
Environment Institute publications

Files in This Item:
File Description SizeFormat 
hdl_56451.pdfPublished version4.68 MBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.