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Neutron Star and Black Hole Binaries in Dense Star Clusters (P7)

Neutron Star and Black Hole Binaries in Dense Star Clusters (P7)

UMASS Amherst Estimation

UMASS Amherst Estimation of binary black hole coalescence event rate exclusion plots with mass and spin parameters from burst search results. Satya Mohapatra and Laura Cadonati Gravitational wave burst sensitivity and event rate upper limit exclusion plots are expressed in terms of root-sumsquared strain amplitudes, hrss: A high mass binary black hole coalescence (> 100 M ) waveform resembles a short duration (10 ms to < 1 s) GW burst. In this poster we estimate the event rate upper limit in binary black hole source parameter space by relating hrss of coalescence waveform with burst search results. GWPAW2011

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