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Fast coalescence of post-Newtonian Supermassive Black Hole Binaries in real galaxies
We present the results of theoretical modeling of supermassive black hole binary (SMBHB) mergers using direct 2 -body simulations with a Hermite integration scheme. The BH’s gravitational interaction is described based on the post-Newtonian (PN-terms) approximation up to the 3.5 PN-terms. We carry o...
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| Main Authors: | , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Головна астрономічна обсерваторія НАН України
2017
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| Series: | Кинематика и физика небесных тел |
| Subjects: | |
| Online Access: | http://dspace.nbuv.gov.ua/handle/123456789/149634 |
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