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We derive the metric on the parameter space of 3.5 post-Newtonian (3.5PN)stationary phase compact binary inspiral waveforms for a single detector,neglecting spin, eccentricity, and finite-body effects. We demonstrate thatthis leads to better template placement than the current practice of using the2PN metric to place 3.5PN templates: The recovered event rate is improved byabout 10% at a cost of nearly doubling the number of templates. Thecross-correlations between mass parameters are also more accurate, which willresult in better coincidence tests.

Parameter space metric for 3.5 post-Newtonian gravitational-waves from compact binary inspirals