{"quality_controlled":"1","scopus_import":"1","month":"01","publication_identifier":{"issn":["2041-8205","2041-8213"]},"publication":"The Astrophysical Journal Letters","year":"2021","doi":"10.3847/2041-8213/abd4d3","oa":1,"volume":907,"_id":"17583","extern":"1","title":"Eccentric black hole mergers in active galactic nuclei","publication_status":"published","abstract":[{"text":"The astrophysical origin of gravitational wave transients is a timely open question in the wake of discoveries by the Laser Interferometer Gravitational-Wave Observatory (LIGO)/Virgo. In active galactic nuclei (AGNs), binaries form and evolve efficiently by interaction with a dense population of stars and the gaseous AGN disk. Previous studies have shown that stellar-mass black hole (BH) mergers in such environments can explain the merger rate and the number of suspected hierarchical mergers observed by LIGO/Virgo. The binary eccentricity distribution can provide further information to distinguish between astrophysical models. Here we derive the eccentricity distribution of BH mergers in AGN disks. We find that eccentricity is mainly due to binary–single (BS) interactions, which lead to most BH mergers in AGN disks having a significant eccentricity at 0.01 Hz, detectable by the Laser Interferometer Space Antenna. If BS interactions occur in isotropic-3D directions, then 8%–30% of the mergers in AGN disks will have eccentricities at 10 Hz above e10 Hz ≳ 0.03, detectable by LIGO/Virgo/Kamioka Gravitational Wave Detector, while 5%–17% of mergers have e10 Hz ≥ 0.3. On the other hand, if BS interactions are confined to the AGN–disk plane due to torques from the disk, with 1–20 intermediate binary states during each interaction, or if BHs can migrate to ≲ 10−3 pc from the central supermassive BH, then 10%–70% of the mergers will be highly eccentric (e10 Hz ≥ 0.3), consistent with the possible high eccentricity in GW190521.","lang":"eng"}],"intvolume":"       907","article_processing_charge":"No","day":"21","status":"public","main_file_link":[{"url":"https://doi.org/10.3847/2041-8213/abd4d3","open_access":"1"}],"date_published":"2021-01-21T00:00:00Z","article_type":"original","language":[{"iso":"eng"}],"issue":"1","author":[{"last_name":"Tagawa","first_name":"Hiromichi","full_name":"Tagawa, Hiromichi"},{"last_name":"Kocsis","full_name":"Kocsis, Bence","first_name":"Bence"},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"last_name":"Bartos","first_name":"Imre","full_name":"Bartos, Imre"},{"last_name":"Omukai","first_name":"Kazuyuki","full_name":"Omukai, Kazuyuki"},{"last_name":"Samsing","first_name":"Johan","full_name":"Samsing, Johan"}],"date_created":"2024-09-05T12:27:07Z","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","type":"journal_article","publisher":"American Astronomical Society","oa_version":"Published Version","citation":{"mla":"Tagawa, Hiromichi, et al. “Eccentric Black Hole Mergers in Active Galactic Nuclei.” <i>The Astrophysical Journal Letters</i>, vol. 907, no. 1, L20, American Astronomical Society, 2021, doi:<a href=\"https://doi.org/10.3847/2041-8213/abd4d3\">10.3847/2041-8213/abd4d3</a>.","ieee":"H. Tagawa, B. Kocsis, Z. Haiman, I. Bartos, K. Omukai, and J. Samsing, “Eccentric black hole mergers in active galactic nuclei,” <i>The Astrophysical Journal Letters</i>, vol. 907, no. 1. American Astronomical Society, 2021.","ista":"Tagawa H, Kocsis B, Haiman Z, Bartos I, Omukai K, Samsing J. 2021. Eccentric black hole mergers in active galactic nuclei. The Astrophysical Journal Letters. 907(1), L20.","apa":"Tagawa, H., Kocsis, B., Haiman, Z., Bartos, I., Omukai, K., &#38; Samsing, J. (2021). Eccentric black hole mergers in active galactic nuclei. <i>The Astrophysical Journal Letters</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/2041-8213/abd4d3\">https://doi.org/10.3847/2041-8213/abd4d3</a>","chicago":"Tagawa, Hiromichi, Bence Kocsis, Zoltán Haiman, Imre Bartos, Kazuyuki Omukai, and Johan Samsing. “Eccentric Black Hole Mergers in Active Galactic Nuclei.” <i>The Astrophysical Journal Letters</i>. American Astronomical Society, 2021. <a href=\"https://doi.org/10.3847/2041-8213/abd4d3\">https://doi.org/10.3847/2041-8213/abd4d3</a>.","short":"H. Tagawa, B. Kocsis, Z. Haiman, I. Bartos, K. Omukai, J. Samsing, The Astrophysical Journal Letters 907 (2021).","ama":"Tagawa H, Kocsis B, Haiman Z, Bartos I, Omukai K, Samsing J. Eccentric black hole mergers in active galactic nuclei. <i>The Astrophysical Journal Letters</i>. 2021;907(1). doi:<a href=\"https://doi.org/10.3847/2041-8213/abd4d3\">10.3847/2041-8213/abd4d3</a>"},"date_updated":"2024-09-19T11:41:11Z","article_number":"L20"}