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In my previous Blog post I have shown the smooth orbit of a single particle around a single, isolated black hole. I have since developed the algorithm for the orbit of a test particle around a pair of identical, non-rotating black holes, in circular orbit around each other.

The pretty chaotic 3 dimensional orbit is shown in on the left. The holes started on the x-axis and the black arrows on the circle indicate their final positions. The particle started at the red arrow and entered a pseudo orbit around the right-hand black hole (on left-hand image), into which it eventually falls after about 2.2 orbits of the black holes around each other.
The dimensions of the plot are: The black holes are separated by D = 50Rs, where Rs = 2GM/(rc2) and M is the mass of each black hole. The holes orbit at a constant speed of Vo = √[M/(2D)] = 0.0707c. The particle starts at x = 25Rs, y = z = -15Rs, with a velocity vector tweaked to produce an interesting (chaotic) orbit. If the particle's speed were 20% more, it would have quickly escaped from the binary holes due to a gravity-assist flyby effect from the right-hand hole, despite the fact that it started at below escape velocity. If its speed were 20% less, it would have quickly been swallowed by the right-hand hole.
Readers are welcome to question me on the issues around binary black holes. I'll answer as far as I'm capable of - I'm still learning this scenario myself...
Jorrie
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