tutorial example code: CDG_gd_Galaxy_imf_se.pyΒΆ

[source code]

   Nbody integration of N particles in N-body units from t=0 to
   t_end=1 N-body time units.  The initial cluster is a King (1966)
   model with dimension-less depth of the potential of W0=7. The
   initial distribution of stars is in virial equilibrium.  At this
   moment a 4th order Hermite integrator is used for the integration.

from amuse.lab import *
from amuse.couple import bridge
from galaxy_model import MilkyWay_galaxy

def main(Ncl, rcl, W0, Rgal, vgal, t_end, n_steps):

    masses = new_salpeter_mass_distribution(Ncl, 1|units.MSun, 100|units.MSun)
    converter = nbody_system.nbody_to_si(masses.sum(), rcl)
    bodies = new_king_model(Ncl, W0, convert_nbody=converter)
    bodies.mass = masses

    stellar = SeBa()
    channel_from_stellar_to_framework = stellar.particles.new_channel_to(bodies)

    bodies.x += Rgal
    bodies.vy += vgal

    CDG = BHTree(converter)
    channel_from_gravity_to_framework = CDG.particles.new_channel_to(bodies)

    gravity = bridge.Bridge()
    gravity.add_system(CDG, (MilkyWay_galaxy(),) )
    dt = t_end/float(n_steps)
    gravity.timestep = dt

    write_set_to_file(bodies.savepoint(0.0 | t_end.unit), filename, "hdf5", append_to_file=False)

    Etot_init = gravity.kinetic_energy + gravity.potential_energy
    Etot_prev = Etot_init

    time = zero
    dt = t_end/float(n_steps)
    while time < t_end:
        time += dt


        write_set_to_file(bodies.savepoint(time), filename, "hdf5")

        Ekin = gravity.kinetic_energy
        Epot = gravity.potential_energy
        Etot = Ekin + Epot
        print "T=", time, "M=", bodies.mass.sum(),
        print "E= ", Etot, "Q= ", Ekin/Epot,
        print "dE=", (Etot_init-Etot)/Etot, "ddE=", (Etot_prev-Etot)/Etot
        Etot_prev = Etot


def new_option_parser():

    from amuse.units.optparse import OptionParser
    result = OptionParser()
    result.add_option("-N", dest="Ncl", type="int",default = 100,
                      help="number of stars [%default]")
    result.add_option("-t", unit=units.Gyr,
                      dest="t_end", type="float", default = 1|units.Gyr,
                      help="end time of the simulation [%default]")
    result.add_option("-n", dest="n_steps", type="float", default = 300,
                      help="number of diagnostics output steps [%default]")
    result.add_option("-r", unit=units.parsec,
                      dest="rcl", type="float", default = 100|units.parsec,
                      help="cluster half-mass radius [%default]")
    result.add_option("-R", unit=units.kpc,
                      dest="Rgal", type="float", default = 8.5|units.kpc,
                      help="distance to the GC [%default]")
    result.add_option("-v", unit=units.kms,
                      dest="vgal", type="float", default = 100|units.kms,
                      help="orbital velocity of the CDG [%default]")
    result.add_option("-W", dest="W0", type="float", default = 7.0,
                      help="Dimension-less depth of the King potential (W0) [%default]")
    return result

if __name__ in ('__main__', '__plot__'):
    set_printing_strategy("custom", #nbody_converter = converter,
                          preferred_units = [units.MSun, units.parsec, units.Myr],
                          precision = 4, prefix = "",
                          separator = " [", suffix = "]")
    o, arguments  = new_option_parser().parse_args()

Keywords: python, amuse, astrophysics, matplotlib, pylab, example, codex (see how-to-search-examples)

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