simple example code: orbit_in_potential.pyΒΆ

(Source code, png, hires.png, pdf)

Integrates a stellar orbit in the galactic potential

This example illustrates the use of a simple external potential and simple integrator, no
amuse community code is used.

import numpy
from amuse.units.optparse import OptionParser
from math import atan
from math import log
from amuse.lab import *
from matplotlib import pyplot
from amuse.plot import plot

class MilkyWay_galaxy(object):
    def __init__(self,potential="point_particle", M=1.6e10 | units.MSun):
        print("pot=", potential)
        if potential.find("Milky")>=0:
            print("Milky Way Potential")
            self.potential = self.Milky_Way_potential
            self.potential = self.point_particle_potential
        self.M = M

    #Generic function to get gravity at a point given the potential
    def get_gravity_at_point(self, pos):
        phi_0 = self.get_potential_at_point(pos)
        grav = AdaptingVectorQuantity()
        dpos = 0.001*pos.length()
        for ii in range(len(pos)):
            ppos = 1.0*pos
            ppos[ii] += dpos
            phi_1 = self.get_potential_at_point(ppos)
            grav.append((phi_1 - phi_0)/dpos)
        return grav

    def get_potential_at_point(self, pos):
        phi = self.potential(pos)
        return phi

    def point_particle_potential(self, pos):
        return self.Kepler_potential(self.M, pos)

    def Kepler_potential(self, mass, pos, eps2=0.0|units.kpc**2):
        return self.Power_law_potential(mass, pos, eps2=eps2, eta=1)

    def Power_law_potential(self, mass, pos, eps2=0.0|units.kpc**2, eta=1):
        return constants.G*mass/(pos.length()**2+eps2)**(eta/2.)

    def disk_and_bulge_potentials(self, pos, a, b, mass):
        r = (pos.x**2+pos.y**2).sqrt()
        return constants.G * mass /\
            (r**2 + (a + (pos.z**2 + b**2).sqrt())**2).sqrt()

    def halo_potential(self, pos, Mc=5.0E+10|units.MSun, Rc=1.0|units.kpc**2):
        r = pos.length()
        rr = (r/Rc)
        return -constants.G * (Mc/Rc)*(0.5*log(1 +rr**2) + atan(rr)/rr)

    def Milky_Way_potential(self, pos):
        pot_disk = self.disk_and_bulge_potentials(pos,
        pot_bulge = self.disk_and_bulge_potentials(pos, 3.7|units.kpc,
        pot_halo = self.halo_potential(pos, Mc=5.0E+10|units.MSun,
        return pot_disk + pot_bulge + pot_halo

def new_single_star(mass, pos, vel):
    single_star = Particle()
    single_star.mass = mass
    single_star.position = pos
    single_star.velocity = vel
    single_star.radius = 1.0 | units.RSun
    return single_star

def evolve_particle_in_potential(single_star, potential, t_end):
    time = 0 | units.Myr
    dt_min = 0.1*t_end
    while time < t_end:
        acc = potential.get_gravity_at_point(single_star.position)
        dt = min(dt_min, 0.1*single_star.velocity.length()/acc.length())
        single_star.velocity += acc*dt
        single_star.position += single_star.velocity*dt
        time += dt

def evolve_particle_trajectory_in_potential(single_star, potential, dt_diag, t_end):
    time = 0 | units.Myr
    x = [] | size_unit
    y = [] | size_unit
    z = [] | size_unit
    while time < t_end:
        evolve_particle_in_potential(single_star, potential, dt_diag)
        time += dt_diag
        print("time=", time, single_star.position.length().as_quantity_in(units.AU))
    return x, y, z

def plot_orbit(x, y):

def new_option_parser():
    result = OptionParser()
    result.add_option("-t", dest="t_end", type="float",default = 250,
                      unit = units.Myr, help="end time [%unit]")
    result.add_option("-d", dest="dt_diag", type="float",default = 10,
                      unit = units.Myr, help="diagnostic timestep [%unit]")
    result.add_option("-P", dest="potential", default = "MilkyWay",
                      help="name of potential")
    result.add_option("-M", dest="mass", type="float",default = 1.e+11,
                      unit = units.MSun, help="mass of the galaxy [%unit]")
    result.add_option("-e", dest="eps", type="float",default = 0.0,
                      unit = units.parsec, help="softening of the potential [%unit]")
    result.add_option("-x", dest="x", type="float",default = 8500,
                      unit = units.parsec, help="x-position [%unit]")
    result.add_option("-y", dest="y", type="float",default = 0,
                      unit = units.parsec, help="y-position [%unit]")
    result.add_option("-z", dest="z", type="float",default = 0,
                      unit = units.parsec, help="z-position [%unit]")
    result.add_option("--vx", dest="vx", type="float",default = 0,
                      unit =,help="x-velocity [%unit]")
    result.add_option("--vy", dest="vy", type="float",default = 220,
                      unit =,help="y-velocity [%unit]")
    result.add_option("--vz", dest="vz", type="float",default = 0,
                      unit =, help="z-velocity [%unit]")
    return result

if __name__ == "__main__":
    o, arguments  = new_option_parser().parse_args()

    t_end = o.t_end
    dt_diag = min(o.dt_diag, 0.1*o.t_end)
    size_unit = units.parsec
    mass = 1.0
    pos = [o.x, o.y, o.z]
    vel = [o.vx, o.vy, o.vz]
    single_star = new_single_star(mass, pos, vel)
    galaxy=MilkyWay_galaxy(o.potential, M=o.mass)
    x, y, z = evolve_particle_trajectory_in_potential(single_star, galaxy, dt_diag, t_end)

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

This Page