In this work we present a dynamical study of IMBHs in which we aim to shed more light on the formation scenario of these objects and on the creation of IMBH binaries (IMBHBs) in young massive star clusters. Specifically, we simulated 10^4 three-body interactions between a binary black hole (BBH) and a massive 60Msol black hole (BH) with ARWV, a direct N-body code that exploits the Mikkola's algorithm for regularization, post-Newtonian parameters up to the 2.5 order and a relativistic kick prescription for mergers.
Dynamical Formation of Intermediate-Mass Black Hole Binaries
Dall'Amico, Marco
2020/2021
Abstract
In this work we present a dynamical study of IMBHs in which we aim to shed more light on the formation scenario of these objects and on the creation of IMBH binaries (IMBHBs) in young massive star clusters. Specifically, we simulated 10^4 three-body interactions between a binary black hole (BBH) and a massive 60Msol black hole (BH) with ARWV, a direct N-body code that exploits the Mikkola's algorithm for regularization, post-Newtonian parameters up to the 2.5 order and a relativistic kick prescription for mergers.File in questo prodotto:
| File | Dimensione | Formato | |
|---|---|---|---|
|
Tesi_LM_Physics_Dall_Amico_Marco.pdf
accesso aperto
Dimensione
6.17 MB
Formato
Adobe PDF
|
6.17 MB | Adobe PDF | Visualizza/Apri |
The text of this website © Università degli studi di Padova. Full Text are published under a non-exclusive license. Metadata are under a CC0 License
Utilizza questo identificativo per citare o creare un link a questo documento:
https://hdl.handle.net/20.500.12608/21288