Table 2
Overview of the suitability of gravitational dynamics solvers for different gravitational regimes.
Code | Small N | Intermediate N | Large N | Large N | Centrally dominated | Post-Newtonian |
(collisional) | (collisional) | (collisional) | (collisionless) | |||
|
||||||
Hermite0 | + | + | ° | ° | ° | − |
PhiGRAPE | + | + | + | ° | ° | − |
ph4 | + | + | + | ° | ° | − |
BHTree | − | − | − | + | − | − |
Octgrav | − | − | − | + | − | − |
Bonsai | − | − | − | + | − | − |
Twobody | N = 2 | − | − | − | + | − |
Huayno | + | + | + | ° | ° | − |
SmallN | + | − | − | − | − | − |
Mercury | − | − | − | − | + | − |
Mikkola | + | − | − | − | − | + |
MI6 | + | + | + | − | + | + |
Pikachu | + | + | + | + | − | − |
Brutus | + | − | − | − | + | − |
HiGPUs | − | + | + | ° | − | − |
Tupan | + | + | ° | ° | ° | + |
MMC | − | − | + | − | − | − |
Fi | − | − | − | + | − | − |
Gadget2 | − | − | − | + | − | − |
Notes.A + indicates that a codes is well suited to a particular regime, a − indicates that the code will fail or run very inefficiently, a ° indicates a limited capability; “small N” means a problem with a small number of bodies, N ≈ 2−100, “intermediate N” means N ≈ 100−104, “large N” means N ≳ 104, “collisionless” indicates gravitational dynamics with some form of softening, “collisional” means simulations without softening. “Centrally dominated” means problems were the dynamics is dominated by a massive central object, such as a solar system or cluster with a supermassive black hole. “Post-Newtonian” indicates whether the code includes post-Newtonian correction terms. Note this table does not address special requirements set by the timescales or the dynamic range of a problem, nor the choice of parameters that may affect the solutions.
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