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2007

Gravitational-wave data analysis using binary black-hole waveforms

Ajith, P.

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Coalescing binary black-hole systems are among the most promising sources of gravitational waves for ground-based interferometers.

While the \emph{inspiral} and \emph{ring-down} stages of the binary black-hole coalescence are well-modelled by analytical approximation methods in general relativity, the recent progress in numerical relativity has enabled us to compute accurate waveforms from the \emph{merger} stage also.
This has an important impact on the search for gravitational waves from binary black holes.
In particular, while the current gravitational-wave searches look for each stage of the coalescence separately, combining the results from analytical and numerical relativity enables us to \emph{coherently} search for all three stages using a single template family.

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