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dc.contributor.author
LIGO-Virgo Collabora
dc.contributor.author
강궁원
dc.date.accessioned
2019-08-28T07:41:22Z
dc.date.available
2019-08-28T07:41:22Z
dc.date.issued
2013-02-13
dc.identifier.issn
1550-7998
dc.identifier.uri
https://repository.kisti.re.kr/handle/10580/14183
dc.description.abstract
This paper presents results of an all-sky search for periodic gravitational waves in the frequency range [50,1 190]  Hz and with frequency derivative range of ∼[-20,1.1]×10-10  Hz s-1 for the fifth LIGO science run (S5). The search uses a noncoherent Hough-transform method to combine the information from coherent searches on time scales of about one day. Because these searches are very computationally intensive, they have been carried out with the Einstein at Home volunteer distributed computing project. Postprocessing identifies eight candidate signals: deeper follow-up studies rule them out. Hence, since no gravitational wave signals have been found, we report upper limits on the intrinsic gravitational wave strain amplitude h0. For example, in the 0.5 Hz-wide band at 152.5 Hz, we can exclude the presence of signals with h0 greater than 7.6×10-25 at a 90% confidence level. This search is about a factor 3 more sensitive than the previous Einstein at Home search of early S5 LIGO data.
dc.language
eng
dc.relation.ispartofseries
Physical review. D, Particles, fields, gravitation, and cosmology
dc.title
Einstein@Home all-sky search for periodic gravitational waves in LIGO S5 data
dc.subject.keyword
Einstein at Home
dc.subject.keyword
Gravitational wave
dc.subject.keyword
LIGO
Appears in Collections:
7. KISTI 연구성과 > 학술지 발표논문
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