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When evolving a star cluster with a mass function with the Nbody6++ code, the masses assigned to particles change after some evolve steps. Perhaps this is related to encounters between stars?
While this remains unfixed, Nbody6++ in AMUSE should not be used for simulations with non-equal mass stars.
0.0 s 4.92440516115e+29 kg
6.31138519872e+12 s 4.92440516115e+29 kg
9.46707779808e+12 s 4.92440516115e+29 kg
1.26227703974e+13 s 4.92440516115e+29 kg
1.57784629968e+13 s 4.92440516115e+29 kg
1.89341555962e+13 s 4.92440516115e+29 kg
2.20898481955e+13 s 4.92440516115e+29 kg
2.46737111522e+13 s 1.2953964666e+30 kg # <-- mass changes
2.84012333942e+13 s 1.2953964666e+30 kg
3.15569259936e+13 s 1.2953964666e+30 kg
3.4712618593e+13 s 1.2953964666e+30 kg
3.78683111923e+13 s 1.2953964666e+30 kg
4.10240037917e+13 s 1.2953964666e+30 kg
4.4179696391e+13 s 1.2953964666e+30 kg
4.73353889904e+13 s 1.2953964666e+30 kg
5.04910815898e+13 s 1.2953964666e+30 kg
5.0783942344e+13 s 4.81168215574e+30 kg # <-- mass changes again
5.68024667885e+13 s 4.81168215574e+30 kg
5.99581593878e+13 s 4.81168215574e+30 kg
6.31138519872e+13 s 4.81168215574e+30 kg
The text was updated successfully, but these errors were encountered:
When evolving a star cluster with a mass function with the Nbody6++ code, the masses assigned to particles change after some evolve steps. Perhaps this is related to encounters between stars?
While this remains unfixed, Nbody6++ in AMUSE should not be used for simulations with non-equal mass stars.
E.g.:
prints the following:
The text was updated successfully, but these errors were encountered: