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Eccentric black hole mergers via three-body interactions in young, globular, and nuclear star clusters
Eccentric mergers are a signature of the dynamical formation channel of binary black holes (BBHs) in dense stellar environments and …
Marco Dall'Amico, Michela Mapelli, Stefano Torniamenti, Manuel Arca Sedda
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Eccentric black hole mergers via three-body interactions in young, globular, and nuclear star clusters
GW190521 formation via three-body encounters in young massive star clusters
GW190521 is the most massive binary black hole (BBH) merger observed to date, and its primary component lies in the pair-instability …
Marco Dall'Amico, Michela Mapelli, Ugo Nicolò Di Carlo, Yann Buffanais, Sara Rastello, Filippo Santoliquido, Alessandro Ballone, Manuel Arca Sedda
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