Details
| Originalsprache | Englisch |
|---|---|
| Aufsatznummer | 064061 |
| Seitenumfang | 13 |
| Fachzeitschrift | Physical Review D |
| Jahrgang | 94 |
| Ausgabenummer | 6 |
| Publikationsstatus | Veröffentlicht - 26 Sept. 2016 |
Abstract
We present results of a high-frequency all-sky search for continuous gravitational waves from isolated compact objects in LIGO's fifth science run (S5) data, using the computing power of the Einstein@Home volunteer computing project. This is the only dedicated continuous gravitational wave search that probes this high-frequency range on S5 data. We find no significant candidate signal, so we set 90% confidence level upper limits on continuous gravitational wave strain amplitudes. At the lower end of the search frequency range, around 1250 Hz, the most constraining upper limit is 5.0×10-24, while at the higher end, around 1500 Hz, it is 6.2×10-24. Based on these upper limits, and assuming a fiducial value of the principal moment of inertia of 1038 kg m2, we can exclude objects with ellipticities higher than roughly 2.8×10-7 within 100 pc of Earth with rotation periods between 1.3 and 1.6 milliseconds.
ASJC Scopus Sachgebiete
- Physik und Astronomie (insg.)
- Physik und Astronomie (sonstige)
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in: Physical Review D, Jahrgang 94, Nr. 6, 064061, 26.09.2016.
Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review
}
TY - JOUR
T1 - Results of an all-sky high-frequency Einstein@Home search for continuous gravitational waves in LIGO's fifth science run
AU - Singh, Avneet
AU - Papa, Maria Alessandra
AU - Eggenstein, Heinz Bernd
AU - Zhu, Sylvia
AU - Pletsch, Holger
AU - Allen, Bruce
AU - Bock, Oliver
AU - Maschenchalk, Bernd
AU - Prix, Reinhard
AU - Siemens, Xavier
PY - 2016/9/26
Y1 - 2016/9/26
N2 - We present results of a high-frequency all-sky search for continuous gravitational waves from isolated compact objects in LIGO's fifth science run (S5) data, using the computing power of the Einstein@Home volunteer computing project. This is the only dedicated continuous gravitational wave search that probes this high-frequency range on S5 data. We find no significant candidate signal, so we set 90% confidence level upper limits on continuous gravitational wave strain amplitudes. At the lower end of the search frequency range, around 1250 Hz, the most constraining upper limit is 5.0×10-24, while at the higher end, around 1500 Hz, it is 6.2×10-24. Based on these upper limits, and assuming a fiducial value of the principal moment of inertia of 1038 kg m2, we can exclude objects with ellipticities higher than roughly 2.8×10-7 within 100 pc of Earth with rotation periods between 1.3 and 1.6 milliseconds.
AB - We present results of a high-frequency all-sky search for continuous gravitational waves from isolated compact objects in LIGO's fifth science run (S5) data, using the computing power of the Einstein@Home volunteer computing project. This is the only dedicated continuous gravitational wave search that probes this high-frequency range on S5 data. We find no significant candidate signal, so we set 90% confidence level upper limits on continuous gravitational wave strain amplitudes. At the lower end of the search frequency range, around 1250 Hz, the most constraining upper limit is 5.0×10-24, while at the higher end, around 1500 Hz, it is 6.2×10-24. Based on these upper limits, and assuming a fiducial value of the principal moment of inertia of 1038 kg m2, we can exclude objects with ellipticities higher than roughly 2.8×10-7 within 100 pc of Earth with rotation periods between 1.3 and 1.6 milliseconds.
UR - http://www.scopus.com/inward/record.url?scp=84990855948&partnerID=8YFLogxK
U2 - 10.48550/arXiv.1607.00745
DO - 10.48550/arXiv.1607.00745
M3 - Article
AN - SCOPUS:84990855948
VL - 94
JO - Physical Review D
JF - Physical Review D
SN - 2470-0010
IS - 6
M1 - 064061
ER -