26 February 2003 Distribution of mass ratios in compact object binaries
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Using the Star Track population synthesis code we compute the distribution of masses of merging compact object (black hole or neutron star) binaries. The shape of the mass distribution is sensitive to some parameters governing the stellar binary evolution. We discuss the possibility of constraining stellar evolution models using mass measurements abtained from detection of compact object inspiral with upcoming gravitational-wave observatories.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Tomasz Bulik, Tomasz Bulik, Krzysztof Belczynski, Krzysztof Belczynski, Vicky Kalogera, Vicky Kalogera, } "Distribution of mass ratios in compact object binaries", Proc. SPIE 4856, Gravitational-Wave Detection, (26 February 2003); doi: 10.1117/12.458968; https://doi.org/10.1117/12.458968


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