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• W2014304222 abstract "The Double Pulsar (PSR J0737−3039) is the only neutron star–neutron star (NS–NS) binary in which both NSs have been detectable as radio pulsars. The Double Pulsar has been assumed to dominate the Galactic NS–NS binary merger rate |${cal R}_{rm g}$| among all known systems, solely based on the properties of the first-born, recycled pulsar (PSR J0737−3039A, or A) with an assumption for the beaming correction factor of 6. In this work, we carefully correct observational biases for the second-born, non-recycled pulsar (PSR J0737−0737B, or B) and estimate the contribution from the Double Pulsar on |${cal R}_{rm g}$| using constraints available from both A and B. Observational constraints from the B pulsar favour a small beaming correction factor for A (∼2), which is consistent with a bipolar model. Considering known NS–NS binaries with the best observational constraints, including both A and B, we obtain |${cal R}_{rm g}=21_{-14}^{+28}$| Myr−1 at 95 per cent confidence from our reference model. We expect the detection rate of gravitational waves from NS–NS inspirals for the advanced ground-based gravitational-wave detectors is to be |$8^{+10}_{-5}$| yr−1 at 95 per cent confidence. Within several years, gravitational-wave detections relevant to NS–NS inspirals will provide us useful information to improve pulsar population models." @default.
• W2014304222 created "2016-06-24" @default.
• W2014304222 creator A5017251529 @default.
• W2014304222 creator A5071983894 @default.
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• W2014304222 date "2015-02-10" @default.
• W2014304222 modified "2023-09-24" @default.
• W2014304222 title "Implications of PSR J0737-3039B for the Galactic NS-NS binary merger rate" @default.
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• W2014304222 doi "https://doi.org/10.1093/mnras/stu2729" @default.
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