Web18 de set. de 2024 · Similarly to RLOF-induced mergers, mergers originating from unbound tertiary systems are dominated by NS–MS mergers, particularly for nonzero . The fraction of NS–NS mergers is relatively high at ∼0.25 for , but rapidly decreases with increasing , dropping to ∼0.01 for in the high-mass tertiary case, and to zero (within our statistical … Web13 de ago. de 2024 · The paper is organized as follows. In Section 2, we describe our method to construct mock GW data and detect signatures for hierarchical mergers.We present our main results in Section 3, and give our conclusions in Section 4. 2 METHOD 2.1 Overview. We introduce a mock data set generated by a simple N-body toy model …
Comparing hierarchical black hole mergers in star clusters and …
WebHence, hierarchical mergers can build up IMBHs and also partially fill the PI mass gap between ∼65 and ∼120 M ⊙, explaining the formation of BBHs like GW190521 (e.g. Fragione, Loeb & Rasio 2024b). One of the main challenges of studying hierarchical mergers is the computational cost. WebWe find that the most massive system in this catalog, GW170729, is mostly likely a first-generation merger, having a 4% probability of being a hierarchical merger assuming a 5 … grand view university golf
Signatures of hierarchical mergers in black hole spin and mass ...
Web1 de out. de 2024 · The rapidly growing number of gravitational-wave discoveries by LIGO and Virgo have brought about several surprises (Aasi et al. 2015; Acernese et al. 2015; Abbott et al. 2024).Surprises included the unexpectedly high mass of some of the black holes, suggesting that they may have been formed through hierarchical mergers … Web14 de abr. de 2024 · As hierarchical mergers occur, a secondary population of high-mass, high-spin black holes begins to form alongside the natal population. In our Monte Carlo procedure, the time evolution of the population is reduced to individual time steps, as described in Section 2.2. Web21 de jun. de 2024 · Hierarchical mergers at traps in AGNs will exhibit black hole spins (anti)aligned with the binary's orbital axis, a distinct property from other hierarchical channels. Our results suggest, although not definitively (with odds ratio of ∼1), that LIGO's heaviest merger so far, GW170729, could have originated from this channel. grandview university in iowa address