Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/48819
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.authorAgeev, A.en
dc.contributor.authorAllen, B.en
dc.contributor.authorAmin, R.en
dc.contributor.authorAnderson, S.en
dc.contributor.authorAnderson, W.en
dc.contributor.authorAraya, M.en
dc.contributor.authorArmandula, H.en
dc.contributor.authorAshley, M.en
dc.contributor.authorAsiri, F.en
dc.contributor.authorAufmuth, P.en
dc.contributor.authorAulbert, C.en
dc.contributor.authorBabak, S.en
dc.contributor.authorBalasubramanian, R.en
dc.contributor.authorBallmer, S.en
dc.contributor.authorBarish, B.en
dc.contributor.authorBarker, C.en
dc.contributor.authorBarker, D.en
dc.contributor.authoret al.en
dc.date.issued2005en
dc.identifier.citationPhysical Review. D. Particles, Fields, Gravitation and Cosmology, 2005; 72(8):082001-1-082001-22en
dc.identifier.issn1550-7998en
dc.identifier.issn1550-2368en
dc.identifier.urihttp://hdl.handle.net/2440/48819en
dc.description.abstractWe use 373 hours (≈15 days) of data from the second science run of the LIGO gravitational-wave detectors to search for signals from binary neutron star coalescences within a maximum distance of about 1.5 Mpc, a volume of space which includes the Andromeda Galaxy and other galaxies of the Local Group of galaxies. This analysis requires a signal to be found in data from detectors at the two LIGO sites, according to a set of coincidence criteria. The background (accidental coincidence rate) is determined from the data and is used to judge the significance of event candidates. No inspiral gravitational-wave events were identified in our search. Using a population model which includes the Local Group, we establish an upper limit of less than 47 inspiral events per year per Milky Way equivalent galaxy with 90% confidence for nonspinning binary neutron star systems with component masses between 1 and 3M⊙.en
dc.description.statementofresponsibilityB. Abbott...C. Killow...D. Ottaway...et al., LIGO Scientific Collaborationen
dc.language.isoenen
dc.publisherAmerican Physical Socen
dc.rights©2005 American Physical Societyen
dc.titleSearch for gravitational waves from galactic and extra-galactic binary neutron starsen
dc.typeJournal articleen
dc.identifier.rmid0020083082en
dc.identifier.doi10.1103/PhysRevD.72.082001en
dc.identifier.pubid41686-
pubs.library.collectionPhysics publicationsen
pubs.verification-statusVerifieden
pubs.publication-statusPublisheden
dc.identifier.orcidOttaway, D. [0000-0001-6794-1591]en
Appears in Collections:Physics publications

Files in This Item:
File Description SizeFormat 
hdl_48819.pdfPublished version1.61 MBAdobe PDFView/Open


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