The impact of pair-instability mass loss on the binary black hole mass distribution
The impact of pair-instability mass loss on the binary black hole mass distribution
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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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A population of binary black hole mergers has now been observed in gravitational waves by Advanced LIGO and Virgo. The masses of these black holes appear to show evidence for a pile-up between \(30\)--\(45\) \(M_\odot\) and a cut-off above \(\sim 45\) \(M_\odot\). One possible explanation for such a pile-up and subsequent cut-off are pulsational pa...
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Full title
The impact of pair-instability mass loss on the binary black hole mass distribution
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TN_cdi_proquest_journals_2205102955
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2205102955
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1904.02821
