Impact of star formation inhomogeneities on merger rates and interpretation of LIGO results
R. O'Shaughnessy (1), R. Kopparapu (2), K. Belczynski (3,4) ((1), University of Wisconsin-Milwaukee, (2) Pennsylvania State University, (3), Astronomical Observatory, University of Warsaw, (4) Center for Gravitational, Wave Astronomy, University of Texas at Brownsville)

TL;DR
This paper discusses how inhomogeneities in star formation affect the accuracy of gravitational wave merger rate predictions, highlighting significant systematic errors and the need to incorporate star-forming condition distributions.
Contribution
It demonstrates that neglecting stellar heterogeneities introduces large systematic errors in merger rate estimates and emphasizes the importance of including star-forming condition distributions.
Findings
Merger rate predictions are sensitive to stellar heterogeneities.
Systematic errors of 30-50% can occur without accounting for inhomogeneities.
Few detections can exhaust information if models neglect heterogeneities.
Abstract
Within the next decade, ground based gravitational wave detectors are in principle capable of determining the compact object merger rate per unit volume of the local universe to better than 20% with more than 30 detections. We argue that the stellar models are sensitive to heterogeneities (in age and metallicity at least) in such a way that the predicted merger rates are subject to an additional 30-50% systematic errors unless these heterogeneities are taken into account. Without adding new electromagnetic constraints on massive binary evolution or relying on more information from each merger (e.g., binary masses and spins), as few as the merger detections could exhaust the information available in a naive comparison to merger rate predictions. As a concrete example, we use a nearby-universe catalog to demonstrate that no one tracer of stellar content can constrain merger…
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