Studying and modelling the complete gravitational-wave signal from precessing black hole binaries
The coalescence of two stellar mass black holes is regarded as one of the most promising sources for the first gravitational-wave (GW) detection with ground-based detectors. The current detection strategies, however, rely on theoretical knowledge of the gravitational waveforms. It is therefore cruci...
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Cardiff University
2014
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.620118 |