most citedBlack Hole Binaries in AGN Accretion Discs II: Gas Effects on Black Hole Satellite Scatterings

4 citations · 7 across the 6 of their papers we have counts for

collaborators

6 papers

gr-qc2023

Gargantuan chaotic gravitational three-body systems II. Dependence on angular momentum and astrophysical scale

Tjarda C. N. Boekholt, Simon F. Portegies Zwart

Recently we estimated that about 5 percent of supermassive black hole triple systems are fundamentally unpredictable. These gargantuan chaotic systems are able to exponentially mag…

astro-ph.HE20234 cited

Black Hole Binaries in AGN Accretion Discs II: Gas Effects on Black Hole Satellite Scatterings

Connar Rowan, Henry Whitehead, Tjarda Boekholt +2

The black hole (BH) binaries in active galactic nuclei (AGN) are expected to form mainly through scattering encounters in the ambient gaseous medium. Recent simulations, including…

astro-ph.GA2023

Punctuated chaos and the unpredictability of the Galactic center S-star orbital evolution

Simon Portegies Zwart, Tjarda Boekholt, Douglas Heggie

We investigate the chaotic behavior of the S-star cluster in the Galactic center using precise -body calculations, free from round-off or discretization errors. Our findings rev…

astro-ph.IM2023

Punctuated Chaos and Indeterminism in Self-gravitating Many-body Systems

Tjarda C. N. Boekholt, Simon F. Portegies Zwart, Douglas C. Heggie

Dynamical chaos is a fundamental manifestation of gravity in astrophysical, many-body systems. The spectrum of Lyapunov exponents quantifies the associated exponential response to…

astro-ph.GA20233 cited

Stirred, not shaken: Star cluster survival in the slingshot scenario

D. Matus Carrillo, M. Fellhauer, T. Boekholt +2

We investigate the effects of an oscillating gas filament on the dynamics of its embedded stellar clusters. Motivated by recent observational constraints, we model the host gas fil…

astro-ph.IM2014

On the Reliability of N-body Simulations

Tjarda Boekholt, Simon Portegies Zwart

The general consensus in the N-body community is that statistical results of an ensemble of collisional N-body simulations are accurate, even though individual simulations are not.…