Accuracy of inference on the physics of binary evolution from gravitational-wave observations
Accuracy of inference on the physics of binary evolution from gravitational-wave observations
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
The properties of the population of merging binary black holes encode some of the uncertain physics of the evolution of massive stars in binaries. The binary black hole merger rate and chirp mass distribution are being measured by ground-based gravitational-wave detectors. We consider isolated binary evolution and explore how accurately the physica...
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Accuracy of inference on the physics of binary evolution from gravitational-wave observations
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TN_cdi_proquest_journals_2073876658
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2073876658
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1711.06287