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Final parsec problem of black hole mergers and ultralight dark matter
Hyeonmo Kooa†
, Dongsu Baka,b†
, Inkyu Parka,b
, Sun...
2
II. SIMULATION
In our simulation, we shall treat BHs as point particles with the Newtonian gravity. The post-Newtonian c...
3
−4 −2 0 2 4
−4
−2
0
2
4
[pc]
t = 0.0 [kyr]
−4 −2 0 2 4
−4
−2
0
2
4
t = 50.0 [kyr]
−4 −2 0 2 4
−4
−2
0
2
4
t = 100.0 [kyr...
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