Dynamics around supermassive black holes: Extreme mass-ratio inspirals as gravitational-wave sources
Dynamics around supermassive black holes: Extreme mass-ratio inspirals as gravitational-wave sources
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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
Supermassive black holes and their surrounding dense stellar environments nourish a variety of astrophysical phenomena. We focus on the distribution of stellar-mass black holes around the supermassive black hole and the consequent formation of extreme-mass-ratio inspirals (EMRIs). We derive a steady-state distribution, considering the effects of tw...
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Dynamics around supermassive black holes: Extreme mass-ratio inspirals as gravitational-wave sources
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TN_cdi_proquest_journals_3074214481
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3074214481
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2406.19443
