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The expected chirp mass distribution of observed events for futuregravitational wave detectors is extensively investigated in the presence of anexotic fluid component with an arbitrary equation of state, $-1 \leq \omega_x\equiv p_x/\rho_x < 0$, i.e., the so-called dark energy component. The resultsfor a flat model dominated by a dark energy are compared to those for thestandard flat model dominated by cold dark matter. It is found that for a flatuniverse the chirp mass distribution shows a sensitive dependence on$\omega_x$, which may provide an independent and robust constraint on thecosmic equation of state.Comment: 5 pages, four figures, aa.sty LaTex fil

Determining the cosmic equation of state using future gravitational wave detectors