Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-03-15
Astronomy and Astrophysics
Astrophysics
12 pages, 15 figures, accepted for publication in MNRAS
Scientific paper
10.1111/j.1365-2966.2008.13557.x
We describe a novel N-body code designed for simulations of the central regions of galaxies containing massive black holes. The code incorporates Mikkola's 'algorithmic' chain regularization scheme including post-Newtonian terms up to PN2.5 order. Stars moving beyond the chain are advanced using a fourth-order integrator with forces computed on a GRAPE board. Performance tests confirm that the hybrid code achieves better energy conservation, in less elapsed time, than the standard scheme and that it reproduces the orbits of stars tightly bound to the black hole with high precision. The hybrid code is applied to two sample problems: the effect of finite-N gravitational fluctuations on the orbits of the S-stars; and inspiral of an intermediate-mass black hole into the galactic center.
Gualandris Alessia
Harfst Stefan
Merritt David
Mikkola Seppo
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