Setting upper limits on the strength of periodic gravitational waves from PSR J1939+2134 using the first science data from the GEO 600 and LIGO detectors
作者： B Abbott , Robert Abbott , R Adhikari , A Ageev , B Allen
DOI: 10.1103/PHYSREVD.69.082004
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摘要: Data collected by the GEO 600 and LIGO interferometric gravitational wave detectors during their first observational science run were searched for continuous waves from pulsar J1939+2134 at twice its rotation frequency. Two independent analysis methods used are demonstrated in this paper: a frequency domain method a time method. Both achieve consistent null results, placing new upper limits on strength of pulsar’s emission. A model emission mechanism is to interpret as constraint equatorial ellipticity.
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