本文整理汇总了Python中amuse.community.sse.interface.SSE类的典型用法代码示例。如果您正苦于以下问题:Python SSE类的具体用法?Python SSE怎么用?Python SSE使用的例子?那么, 这里精选的类代码示例或许可以为您提供帮助。
在下文中一共展示了SSE类的15个代码示例,这些例子默认根据受欢迎程度排序。您可以为喜欢或者感觉有用的代码点赞,您的评价将有助于系统推荐出更棒的Python代码示例。
示例1: test16
def test16(self):
print "test evolution of 1000 star sampled over flattish IMF"
number_of_stars=1000
class notsorandom(object):
def random(self,N):
return numpy.array(range(N))/(N-1.)
def random_sample(self,N):
return numpy.array(range(N))/(N-1.)
masses = new_salpeter_mass_distribution(
number_of_stars,
mass_min = 0.1 | units.MSun,
mass_max = 100.0 | units.MSun,
alpha = -1.01,random=notsorandom()
)
stars=Particles(mass=masses)
instance=SSE()
instance.particles.add_particles(stars)
i=0
for p in instance.particles:
print i,p.mass,
p.evolve_for(13.2 | units.Gyr)
print p.mass
i+=1
instance.stop()
示例2: test18
def test18(self):
print "SSE validation"
sse_src_path = os.path.join(os.path.dirname(sys.modules[SSE.__module__].__file__), 'src')
if not os.path.exists(os.path.join(sse_src_path, "evolve.in")):
self.skip("Not in a source release")
instance = SSE()
instance.particles.add_particle(Particle(mass = 1.416 | units.MSun))
instance.particles[0].evolve_for(7000.0 | units.Myr)
evolved_star = instance.particles.copy()[0]
evolved_star.temperature = instance.particles[0].temperature
instance.stop()
testpath = get_path_to_results()
shutil.copy(os.path.join(sse_src_path, "evolve.in"), os.path.join(testpath, "evolve.in"))
call([os.path.join(sse_src_path, "sse")], cwd=testpath)
with open(os.path.join(testpath, "evolve.dat"), "r") as sse_output:
lines = sse_output.readlines()
sse_final_result = lines[-2].split()
self.assertAlmostEqual(evolved_star.age, float(sse_final_result[0]) | units.Myr, 3)
self.assertAlmostEqual(evolved_star.stellar_type, float(sse_final_result[1]) | units.stellar_type, 3)
self.assertAlmostEqual(evolved_star.initial_mass, float(sse_final_result[2]) | units.MSun, 3)
self.assertAlmostEqual(evolved_star.mass, float(sse_final_result[3]) | units.MSun, 3)
self.assertAlmostEqual(evolved_star.luminosity, 10**float(sse_final_result[4]) | units.LSun, 3)
self.assertAlmostEqual(evolved_star.radius, 10**float(sse_final_result[5]) | units.RSun, 3)
self.assertAlmostRelativeEqual(evolved_star.temperature, 10**float(sse_final_result[6]) | units.K, 2)
self.assertAlmostEqual(evolved_star.core_mass, float(sse_final_result[7]) | units.MSun, 3)
self.assertAlmostEqual(evolved_star.convective_envelope_mass, float(sse_final_result[8]) | units.MSun, 3)
self.assertAlmostEqual(evolved_star.epoch, float(sse_final_result[9]) | units.Myr, 3)
self.assertAlmostEqual(evolved_star.spin, float(sse_final_result[10]) | units.yr**-1, 3)
示例3: test17
def test17(self):
print "evolve_one_step and evolve_for after particle removal and addition"
particles = Particles(10)
particles.mass = range(1, 11) | units.MSun
instance = SSE()
instance.particles.add_particles(particles)
self.assertAlmostEqual(instance.particles.age, 0.0 | units.yr)
time_steps = numpy.linspace(0.1, 1.0, num=10) | units.Myr
for i in range(10):
instance.particles[i].evolve_for(time_steps[i])
self.assertAlmostEqual(instance.particles.age, time_steps)
instance.particles.remove_particles(particles[[1, 4, 8]])
revived = instance.particles.add_particle(particles[4])
revived.evolve_for(numpy.pi | units.Myr)
for star in instance.particles:
star.evolve_for(star.age)
self.assertAlmostEqual(instance.particles.age[:-1], 2*time_steps[[0, 2,3, 5,6,7, 9]])
self.assertAlmostEqual(instance.particles.age[-1], 2*numpy.pi | units.Myr)
instance.particles.remove_particles(particles[[2, 5, 6]])
instance.particles.add_particles(particles[[8, 1]])
self.assertEqual(len(instance.particles), 7)
expected_ages = instance.particles.age + instance.particles.time_step
for star in instance.particles:
star.evolve_one_step()
self.assertAlmostEqual(instance.particles.age, expected_ages)
instance.stop()
示例4: simulate_evolution_tracks
def simulate_evolution_tracks():
stellar_evolution = SSE()
star = datamodel.Particle()
star.mass = stellar_mass
star = stellar_evolution.particles.add_particle(star)
luminosity_at_time = [] | units.LSun
temperature_at_time = [] | units.K
print("Evolving a star with mass:", stellar_mass)
is_evolving = True
while is_evolving and star.age < end_time:
luminosity_at_time.append(star.luminosity)
temperature_at_time.append(star.temperature)
previous_age = star.age
# if we do not specify an end_time in the evolve_model function
# a stellar evolution code will evolve to the next
# 'natural' timestep, this will ensure all interesting physics
# is seen in the hr diagram
stellar_evolution.evolve_model()
is_evolving = (star.age != previous_age)
stellar_evolution.stop()
return temperature_at_time, luminosity_at_time
示例5: plottillagb
def plottillagb():
sun = datamodel.Particle(
mass=1 | units.MSun,
radius=1 | units.RSun
)
sse = SSE()
sse.particles.add_particle(sun)
channel_from_se_to_memory = sse.particles.new_channel_to(sun.as_set())
channel_from_se_to_memory.copy()
masses = [] | units.MSun
timerange = numpy.arange(11500, 13500, 10) | units.Myr
for time in timerange:
sse.evolve_model(time)
channel_from_se_to_memory.copy()
masses.append(sun.mass)
print(time.as_quantity_in(units.Myr),
sun.mass.as_quantity_in(units.MSun))
sse.stop()
figure = pyplot.figure(figsize=(6, 6))
subplot = figure.add_subplot(1, 1, 1)
subplot.plot(timerange.value_in(units.Gyr),
masses.value_in(units.MSun), '.')
subplot.set_xlabel('t (Gyr)')
subplot.set_ylabel('mass (MSun)')
pyplot.show()
示例6: test23
def test23(self):
instance = SSE()
p=Particles(mass = [1.0, 10.0] | units.MSun, temperature=[10,10] | units.K)
stars = instance.particles.add_particles(p)
channel=stars.new_channel_to(p)
channel.copy_attributes(["mass","temperature"])
self.assertEqual(stars.temperature, p.temperature)
instance.stop()
示例7: test6
def test6(self):
print "Test whether a set of stars evolves synchronously..."
# Create an array of stars with a range in stellar mass
masses = [.5, 1., 2., 5., 10., 30.] | units.MSun
number_of_stars = len(masses)
stars = Particles(number_of_stars)
stars.mass = masses
# Initialize stellar evolution code
instance = SSE()
instance.commit_parameters()
instance.particles.add_particles(stars)
instance.commit_particles()
from_code_to_model = instance.particles.new_channel_to(stars)
from_code_to_model.copy()
instance.evolve_model(end_time = 125 | units.Myr)
from_code_to_model.copy()
end_types = (
"deeply or fully convective low mass MS star",
"Main Sequence star",
"Main Sequence star",
"Carbon/Oxygen White Dwarf",
"Neutron Star",
"Black Hole",
)
for i in range(number_of_stars):
self.assertAlmostEquals(stars[i].age, 125.0 | units.Myr)
self.assertTrue(stars[i].mass <= masses[i])
self.assertEquals(str(stars[i].stellar_type), end_types[i])
instance.stop()
示例8: test21
def test21(self):
instance = SSE()
stars = instance.particles.add_particles(Particles(mass = 30 | units.MSun))
mass_loss_wind = stars[0].mass_loss_wind
self.assertAlmostRelativeEquals(mass_loss_wind, 1.703e-07 | units.MSun / units.yr, 3)
instance.evolve_model(1 | units.Myr)
dm = (1 | units.Myr)* mass_loss_wind
self.assertAlmostRelativeEquals(stars[0].mass, (30 | units.MSun) - dm , 3)
self.assertAlmostRelativeEquals(stars[0].mass_loss_wind, 2.053e-07 | units.MSun / units.yr, 3)
instance.stop()
示例9: test9
def test9(self):
print "Test: large number of particles"
stellar_evolution = SSE(max_message_length=500)
stellar_evolution.commit_parameters()
number_of_particles = 10000
print "Has been tested with up to a million particles!"
print "Now using ", number_of_particles, "particles only, for speed."
stars = Particles(number_of_particles)
stars.mass = 1.0 | units.MSun
stellar_evolution.particles.add_particles(stars)
self.assertEqual(len(stellar_evolution.particles), number_of_particles)
stellar_evolution.stop()
示例10: stellar_lifetime
def stellar_lifetime(mZAMS, z=0.02):
global se
if se is None:
se = SSE()
se.parameters.metallicity = z
se.particles.add_particle(Particle(mass=mZAMS))
while not stellar_remnant_state(se.particles[0]):
se.evolve_model()
t_end = se.particles[0].age
# tpe = se.particles[0].stellar_type
se.particles.remove_particle(se.particles[0])
return t_end
示例11: test20
def test20(self):
print "SSE core_mass and CO_core_mass (low mass stars)"
instance = SSE()
stars = instance.particles.add_particles(Particles(mass = [0.6, 1.0] | units.MSun))
instance.evolve_model(100 | units.Gyr)
self.assertEqual(str(stars[0].stellar_type), "Helium White Dwarf")
self.assertAlmostEqual(stars[0].mass, 0.405 | units.MSun, 2)
self.assertEqual(stars[0].core_mass, stars[0].mass)
self.assertEqual(stars[0].CO_core_mass, 0 | units.MSun)
self.assertEqual(str(stars[1].stellar_type), "Carbon/Oxygen White Dwarf")
self.assertAlmostEqual(stars[1].mass, 0.520 | units.MSun, 2)
self.assertEqual(stars[1].core_mass, stars[1].mass)
self.assertEqual(stars[1].CO_core_mass, stars[1].mass)
instance.stop()
示例12: test10
def test10(self):
stellar_evolution = SSE()
stellar_evolution.commit_parameters()
stars = Particles(10)
stars.mass = 1.0 | units.MSun
stellar_evolution.particles.add_particles(stars)
self.assertEquals(stellar_evolution.particles._factory_for_new_collection(), Particles)
filename = os.path.join(get_path_to_results(), "test.h5")
if os.path.exists(filename):
os.remove(filename)
io.write_set_to_file(stellar_evolution.particles, filename, 'hdf5')
stored_stars = io.read_set_from_file(filename, 'hdf5')
self.assertEquals(len(stars), len(stored_stars))
self.assertAlmostRelativeEquals(stars.mass, stored_stars.mass)
示例13: test5
def test5(self):
sse = SSE()
sse.commit_parameters()
stars = Particles(1)
star = stars[0]
star.mass = 35 | units.MSun
star.radius = 0.0 | units.RSun
stars.synchronize_to(sse.particles)
channel = sse.particles.new_channel_to(stars)
channel.copy_attributes(sse.particles.get_attribute_names_defined_in_store())
previous_type = star.stellar_type
results = []
dt = 1 | units.Myr
t = 0 | units.Myr
while t < 30 | units.Myr:
t += dt
sse.evolve_model(t)
self.assertTrue(sse.particles[0].mass.value_in(units.MSun) < 10.6)
sse.stop()
示例14: test8
def test8(self):
instance = SSE()
self.assertEqual(instance.parameters.reimers_mass_loss_coefficient, 0.5)
myvalue = 0.7
instance.parameters.reimers_mass_loss_coefficient = myvalue
self.assertEqual(instance.parameters.reimers_mass_loss_coefficient, myvalue)
instance.commit_parameters()
self.assertEqual(instance.parameters.reimers_mass_loss_coefficient, myvalue)
instance.stop()
instance = SSE()
self.assertEqual(instance.parameters.reimers_mass_loss_coefficient, 0.5)
myvalue = 0.7
instance.parameters.reimers_mass_loss_coefficient = myvalue
instance.parameters.set_defaults()
instance.commit_parameters()
self.assertEqual(instance.parameters.reimers_mass_loss_coefficient, 0.5)
instance.stop()
示例15: test14b
def test14b(self):
print "Testing basic operations: evolve_one_step and evolve_for (on subset)"
stars = Particles(2)
stars.mass = 1.0 | units.MSun
instance = SSE()
se_stars = instance.particles.add_particles(stars)
self.assertAlmostEqual(se_stars.age, [0.0, 0.0] | units.yr)
for i in range(3):
se_stars[:1].evolve_one_step()
self.assertAlmostEqual(se_stars.age, [1650.46953688, 0.0] | units.Myr, 3)
number_of_steps = 10
step_size = se_stars[0].age / number_of_steps
for i in range(1, number_of_steps + 1):
se_stars[1:].evolve_for(step_size)
self.assertAlmostEqual(se_stars.age, [number_of_steps, i] * step_size)
print se_stars
self.assertAlmostRelativeEqual(se_stars[0].age, se_stars[1].age)
self.assertAlmostRelativeEqual(se_stars[0].luminosity, se_stars[1].luminosity, 3)
self.assertAlmostRelativeEqual(se_stars[0].radius, se_stars[1].radius, 3)
self.assertAlmostRelativeEqual(se_stars[0].temperature, se_stars[1].temperature, 3)
instance.stop()