Comprehensive all-sky search for periodic gravitational waves in the sixth science run LIGO data

LIGO Scientific Collaboration and Virgo Collaboration

Research output: Contribution to journalArticle

19 Citations (Scopus)

Abstract

We report on a comprehensive all-sky search for periodic gravitational waves in the frequency band 100-1500 Hz and with a frequency time derivative in the range of [-1.18,+1.00]×10-8 Hz/s. Such a signal could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our galaxy. This search uses the data from the initial LIGO sixth science run and covers a larger parameter space with respect to any past search. A Loosely Coherent detection pipeline was applied to follow up weak outliers in both Gaussian (95% recovery rate) and non-Gaussian (75% recovery rate) bands. No gravitational wave signals were observed, and upper limits were placed on their strength. Our smallest upper limit on worst-case (linearly polarized) strain amplitude h0 is 9.7×10-25 near 169 Hz, while at the high end of our frequency range we achieve a worst-case upper limit of 5.5×10-24. Both cases refer to all sky locations and entire range of frequency derivative values.

Original languageEnglish (US)
Article number042002
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume94
Issue number4
DOIs
StatePublished - Aug 15 2016

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LIGO (observatory)
gravitational waves
sky
recovery
metal spinning
neutron stars
frequency ranges
galaxies

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Cite this

Comprehensive all-sky search for periodic gravitational waves in the sixth science run LIGO data. / LIGO Scientific Collaboration and Virgo Collaboration.

In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 94, No. 4, 042002, 15.08.2016.

Research output: Contribution to journalArticle

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