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Delete COSMIC/COSMIC_v3_evolve.py

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Yaël M
2024-06-21 16:22:13 +02:00
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parent d07dd2ed88
commit d87a37bdc5
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COSMIC/COSMIC_v3_evolve.py
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"""
* COSMIC - EVOLVE
* Version 3
@ Yaël Moussouni
@ Unistra, P&E, MSc1-MoFP
@ Observatory of Strasbourg (Intern)
"""
import numpy as np
import amuse.units.units as u
import COSMIC_v3_output as output
import COSMIC_v3_emission as emission
import COSMIC_v3_coordinates as coords
def stellar_gravity(codes, stars, channels, params, save_stars = False):
"""
Evolve a model with both gravity and stellar evolution.
"""
for t in params["output_times"]:
print("\033[36m"+"t: "+"\033[0m"+"{:02.2f} Myr/{:02.2f} Myr".format(t.value_in(u.Myr),np.max(params["output_times"].value_in(u.Myr))))
codes["g"].evolve_model(t)
channels.copy()
if save_stars: output.save_stars(stars, params, t.value_in(u.Myr))
print("\033[36m"+"Simulation completed"+"\033[0m")
return 0
def stellar_gravity_binaries(codes, stars, binaries, channels, params, save_stars = False, save_binaries = False, compute_X_emission = False):
"""
Evolve a model with both gravity and stellar evolution.
"""
for t in params["output_times"]:
print("\033[36m"+"t: "+"\033[0m"+"{:02.2f} Myr/{:02.2f} Myr".format(t.value_in(u.Myr),np.max(params["output_times"].value_in(u.Myr))))
codes["b"].evolve_model(t)
channels.copy()
stars = coords.xyz2radecdist(stars)
if compute_X_emission:
stars = emission.rotation(stars, params)
stars = emission.X_emission(stars, params)
stars = emission.plasma_temperature(stars, params)
if save_stars: output.save_stars(stars, params, t.value_in(u.Myr))
if save_binaries: output.save_binaries(binaries, params, t.value_in(u.Myr))
print("\033[36m"+"Simulation completed"+"\033[0m")
return codes, stars, channels