Upper Limits on the Stochastic Background of Gravitational Waves

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dc.contributor.authorMcClelland, David
dc.contributor.authorScott, Susan M
dc.contributor.authorSearle, Antony
dc.contributor.authorWette, Karl
dc.contributor.authorHeefner, J
dc.contributor.authorHough, J
dc.contributor.authorIvanov, A
dc.date.accessioned2015-12-13T22:54:32Z
dc.date.issued2005
dc.date.updated2016-06-14T08:37:02Z
dc.description.abstractThe Laser Interferometer Gravitational-Wave Observatory has performed a third science run with much improved sensitivities of all three interferometers. We present an analysis of approximately 200 hours of data acquired during this run, used to search for a stochastic background of gravitational radiation. We place upper bounds on the energy density stored as gravitational radiation for three different spectral power laws. For the flat spectrum, our limit of 0 < 8.4 × 10 -4 in the 69-156 Hz band is ∼10 5 times lower than the previous result in this frequency range.
dc.identifier.issn0031-9007
dc.identifier.urihttp://hdl.handle.net/1885/82150
dc.publisherAmerican Physical Society
dc.sourcePhysical Review Letters
dc.subjectKeywords: Energy density; Frequency ranges; Gravitational radiation; Gravitational waves; Laser interferometer gravitational-wave observatories; Spectral power laws; Upper Bound; Upper limits; Gravity waves; Interferometers; Laser interferometry; Radiation; Stochas
dc.titleUpper Limits on the Stochastic Background of Gravitational Waves
dc.typeJournal article
local.bibliographicCitation.lastpage6
local.bibliographicCitation.startpage221101/1
local.contributor.affiliationMcClelland, David, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationScott, Susan M, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSearle, Antony, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationWette, Karl, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationHeefner, J, California Institute of Technology
local.contributor.affiliationHough, J, University of Glasgow
local.contributor.affiliationIvanov, A, California Institute of Technology
local.contributor.authoruidMcClelland, David, u8802403
local.contributor.authoruidScott, Susan M, u8911327
local.contributor.authoruidSearle, Antony, u9719170
local.contributor.authoruidWette, Karl, u4090078
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.absfor029904 - Synchrotrons; Accelerators; Instruments and Techniques
local.identifier.ariespublicationMigratedxPub10433
local.identifier.citationvolume95
local.identifier.doi10.1103/PhysRevLett.95.221101
local.identifier.scopusID2-s2.0-76249096276
local.type.statusPublished Version

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