Searching for gravitational waves emitted by binaries with spinning components
作者： Gareth Jones
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摘要: In this thesis we consider the data analysis problem of detecting gravitational waves emitted by inspiraling binary systems. Detection will open a new window on Universe enabling direct detection systems such as black holes for first time. Chapter show how are derived from Einstein's General theory Relativity and discuss emission binaries radiation may be detected using laser interferometers. Around two thirds stars inhabit As they orbit each other emit both energy angular momentum in form which inevitably lead to their inspiral eventual merger. To date, searches during have concentrated with non-spinning components. 2 detail dedicated search consisting spinning stellar mass compact objects. We analysed 788 hours collected third science run (S3) LIGO detectors, no was made set an upper limit rate coalescences binaries. The objects into super massive radiate at frequencies detectable planned space-based LISA mission. 3 describe development testing computationally cheap method detect loudest few extreme ratio events that sensitive to.
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