Probability distribution function for inclinations of merging compact binaries detected by gravitational wave interferometers

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Abstract

We analytically discuss probability distribution functions (PDFs) for inclinations of merging compact binaries whose gravitational waves are coherently detected by a network of ground-based interferometers. These PDFs would be useful for studying the possibility of (1) simultaneously detecting electromagnetic signals (such as gamma-ray bursts) associated with binary mergers and (2) statistically constraining the related theoretical models using actual observational data frommulti-messenger astronomy. Our approach is similar to Schutz (2011), but we explicitly include the dependence of the polarization angles of the binaries, based on the concise formulation given in Cutler & Flanagan (1994). We find that the overall profiles of the PDFs are similar for any network of second-generation detectors (Advanced-LIGO, Advanced-Virgo, KAGRA and LIGO-India). For example, 5.1 per cent of detected binaries would have inclination angle less than 10° with at most 0.1 per cent differences between the potential networks. A perturbative expression is also provided for generating the PDFs with a small number of parameters given by directional averages of the quantity ε that characterizes the asymmetry of network sensitivities to two incoming orthogonal polarization modes.

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Seto, N. (2015). Probability distribution function for inclinations of merging compact binaries detected by gravitational wave interferometers. Monthly Notices of the Royal Astronomical Society, 446(3), 2887–2894. https://doi.org/10.1093/mnras/stu2183

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