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• W3204181388 abstract "Since the initial detection of gravitational waves in 2015, over 50 candidate events have been reported by the LIGO-Virgo-KAGRA collaboration. As the current generation of detectors move toward their design sensitivity, the rate of these detections will increase. The next generation of detectors are likely to have high enough sensitivities that multiple merging binaries will be visible at the same time. In this paper we show that this is likely to happen before the end of the decade, during observations by the LIGO-Voyager detector. We investigate the situation of overlapping binary black hole (BBH) mergers in these detectors. We find that current parameter estimation techniques are capable of distinguishing the louder of two merging BBH events, without significant bias, when their merger times are not less than $ensuremath{sim}0.1$ seconds apart or when the ratio of the signal-to-noise ratios of the systems is uneven. This region of overlapping parameter space is dependent upon the sky locations of the signals and the relation of those locations to the light travel time between detectors. We also find that, if two signals are highly overlapping, then the recovered set of parameters often show strong evidence of precession. Finally, we show that bias can occur even when the signal causing the bias is below the detection threshold." @default.
• W3204181388 created "2021-10-11" @default.
• W3204181388 creator A5045344676 @default.
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• W3204181388 date "2021-10-08" @default.
• W3204181388 modified "2023-10-16" @default.
• W3204181388 title "Parameter estimation bias from overlapping binary black hole events in second generation interferometers" @default.
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• W3204181388 doi "https://doi.org/10.1103/physrevd.104.084039" @default.
• W3204181388 hasPublicationYear "2021" @default.
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