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MakeCloud_Bondi.py
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MakeCloud_Bondi.py
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#!/usr/bin/env python
"""
MakeCloud: "Believe me, we've got some very turbulent clouds, the best clouds. You're gonna love it."
This is an alternate version that creates a homogeneous spherical medium around a sink particle, meant to do a Bondi-accretion test. By default it uses default GIZMO units
Usage: MakeCloud_Bondi.py [options]
Options:
-h --help Show this screen.
--R_over_Rsonic=<f> Outer radius of the cloud in Rsonic [default: 16.0]
--Rs_over_Rsonic=<f> Ratio of sink radius to sonic radius [default: 1.0]
--rho_gas=<msun> Density of the gas around the sink at inifinity, in msolar/pc^3 [default: 0.01]
--filename=<name> Name of the IC file to be generated
--N=<N> Number of gas particles [default: 583200]
--MBH=<msun> Mass of the sink at center of the sphere, should be much larger than the gas mass, in msolar [default: 1.0]
--boxsize=<f> Simulation box size in pc
--length_unit=<pc> Unit of length in pc [default: 1000]
--mass_unit=<msun> Unit of mass in M_sun [default: 1e10]
--v_unit=<m/s> Unit of velocity in m/s [default: 1000]
--GMC_units Sets units appropriate for GMCs, so pc, m/s, m_sun, tesla
--localdir Changes directory defaults assuming all files are used from local directory.
--R_cut_out=<f> Distance around the sink to be left empty in pc [default: 0.0001]
"""
from __future__ import print_function
import numpy as np
from scipy import fftpack, interpolate, ndimage
from scipy.integrate import quad, odeint, solve_bvp
from scipy.spatial import cKDTree
from scipy.spatial.distance import cdist
from scipy.optimize import minimize
import sys
import h5py
import os
from docopt import docopt
# from pykdgrav import Potential
arguments = docopt(__doc__)
GMC_units = arguments["--GMC_units"]
length_unit = float(arguments["--length_unit"])
mass_unit = float(arguments["--mass_unit"])
v_unit = float(arguments["--v_unit"])
if GMC_units:
length_unit = 1.0
mass_unit = 1.0
v_unit = 1.0
R_over_Rsonic = float(arguments["--R_over_Rsonic"])
Rs_over_Rsonic = float(arguments["--Rs_over_Rsonic"])
rho_gas = float(arguments["--rho_gas"]) / (
mass_unit / (length_unit**3.0)
) # msolar/pc^3 to code units
N_gas = int(float(arguments["--N"]) + 0.5)
M_BH = float(arguments["--MBH"]) / mass_unit # mstar to code units
R_cut_out = float(arguments["--R_cut_out"]) / length_unit
filename = arguments["--filename"]
localdir = arguments["--localdir"]
# set gravitational constant
G = 4325.69 / length_unit / (v_unit**2) * (mass_unit)
if localdir:
turb_path = "turb"
glass_path = "glass_256.npy"
# get rsink radius from sonic radius
csound = 200 / v_unit # 200 m/s
rsonic_Bondi = G * M_BH / 2.0 / (csound**2) / length_unit
msonic = 4.0 * np.pi / 3.0 * rho_gas * (rsonic_Bondi**3.0)
Rsink = Rs_over_Rsonic * rsonic_Bondi
R = R_over_Rsonic * rsonic_Bondi
print("Radius set as %g pc" % (R * length_unit))
if arguments["--boxsize"] is not None:
# print((arguments["--boxsize"]))
boxsize = float(arguments["--boxsize"]) * length_unit
else:
boxsize = 10 * R
center = np.ones(3) * boxsize / 2.0
res_effective = int(N_gas ** (1.0 / 3.0) + 0.5)
# Load Bondi Spherical solution
IC_data = np.loadtxt("BONDI_SOLUTION.dat") # load IC data from Hubber
data_r = IC_data[:, 0] * rsonic_Bondi # coordinate originally in Rsonic
data_within_R_index = data_r <= R
data_r = data_r[data_within_R_index] # restrict to within R radius
data_mass_in_r = (
IC_data[data_within_R_index, 1] * msonic
) # gas mass in units of 4*pi*rho0*Rsonic^3/3
data_density = (
IC_data[data_within_R_index, 2] * rho_gas
) # density originally in rho0
data_vr = (
IC_data[data_within_R_index, 3] * csound
) # velocity originally in csound
M_gas = np.max(data_mass_in_r) # normalize to total mass
# Get glass
mgas = np.repeat(M_gas / N_gas, N_gas) # gas mass init
x = 2 * (np.load(glass_path) - 0.5) # load glass to have basic structure
Nx = len(x[:, 0])
# original glass size
r = np.sum(x**2, axis=1) ** 0.5 # calculate radius
x = x[r.argsort()][
:N_gas
] # sort the particles by radius, it should be spherically symmetric, now take the right number of particles
x *= (float(Nx) / N_gas * 4 * np.pi / 3 / 8) ** (
1.0 / 3
) # scale up the sphere to have unit radius
r = np.sum(x**2, axis=1) ** 0.5 # recalculate radius
# Strech the particles based on how much mass is in a given radius
int_mass = np.cumsum(mgas) # integrated mass
newr = np.interp(
int_mass, data_mass_in_r, data_r
) # calculate the radius the particles should be at to have the sane mass within the radius a sthe solution
stretch = newr / r # stretch factor
x[:, 0] *= stretch
x[:, 1] *= stretch
x[:, 2] *= stretch
u = (
np.ones_like(mgas) * 0.101 * ((1000 / v_unit) ** 2) / 2.0
) # /2 needed because it is molecular
rho = np.interp(
int_mass, data_mass_in_r, data_density
) # interpolate the density
h = (32 * mgas / rho) ** (1.0 / 3)
vr = np.interp(int_mass, data_mass_in_r, data_vr) # interpolate the velocity
v = -x
v[:, 0] *= vr / newr
v[:, 1] *= vr / newr
v[:, 2] *= vr / newr
# print chek data
print(
"mdot avg: %g std %g"
% (
np.mean(data_density * data_r * data_r * data_vr * np.pi * 4.0),
np.std(data_density * data_r * data_r * data_vr * np.pi * 4.0),
)
)
print("density")
print(data_density)
print("density_alt")
altdens = (
np.diff(data_mass_in_r)
/ np.diff(data_r)
/ (4.0 * np.pi * data_r[1:] * data_r[1:])
)
print(altdens)
print("relative")
print(data_density[1:] / altdens)
# Calculate NEWSNK parameters
print("Calculating t_radial...")
for z in [0.125, 0.5, 1.0, 2.0, 4.0]:
print("\t At %g Rsonic = %g pc" % (z, (rsonic_Bondi * z * length_unit)))
ind = newr <= (z * rsonic_Bondi)
print("\t mass enclosed %g in msun" % (np.sum(mgas[ind]) * mass_unit))
# tot_weight=np.sum(mgas[ind]/rho[ind])
tot_weight = 4.0 / 3.0 * np.pi * np.max(newr[ind]) ** 3
x_dot_v = np.sum(x * v, axis=1)
t_rad = (
-np.sum(mgas[ind])
* tot_weight
/ np.sum(4.0 * np.pi * (x_dot_v * newr * mgas)[ind])
)
print("\t t_rad=%g in code units" % (t_rad))
print("\t m/t_rad=%g in code units" % (np.sum(mgas[ind]) / t_rad))
# from IC
ind = np.arange(len(data_r))[(data_r <= (z * rsonic_Bondi))]
ind2 = np.argmax(data_r[ind])
dm_ic = np.diff(data_mass_in_r)
t_rad_IC = (
data_mass_in_r[ind2] * (4.0 / 3.0 * np.pi) * data_r[ind2] ** 3
) / (
4.0
* np.pi
* np.sum(data_r[ind] * data_r[ind] * data_vr[ind] * dm_ic[ind])
)
print("\t t_rad_IC=%g in code units" % (t_rad_IC))
print(
"\t m_IC/t_rad_IC=%g in code units" % (data_mass_in_r[ind2] / t_rad_IC)
)
# Calculate flux
print("Calculating density ...")
dr = np.diff(newr)
rho_alt = (mgas[1:] / dr) / (4.0 * np.pi * (newr[1:] ** 2))
print(rho)
print(rho_alt)
print(rho[1:] / rho_alt)
# keep the one sthat are not too close
ind = newr > R_cut_out
print(
"Removing %d particles that are inside R_cut_out of %g"
% ((N_gas - np.sum(ind)), R_cut_out)
)
N_gas = np.sum(ind)
M_gas = np.sum(mgas[ind])
NGBvals = [1, 2, 5, 10, 20, 50, 100, 200, 400, 800, 1600]
for ngb in NGBvals:
print("Radius at Ngbfactor of %g is %g pc" % (ngb, newr[32 * ngb]))
# center coordinates
x = x + boxsize / 2.0
print("Writing snapshot...")
if filename is None:
filename = (
"rho%3.2g_" % (rho_gas * (mass_unit / (length_unit**3)))
+ ("MBH%g_" % (mass_unit * M_BH) if M_BH > 0 else "")
+ "R_over_Rsonic%g_Res%d_Rs_over_Rsonic%g"
% (R_over_Rsonic, res_effective, Rs_over_Rsonic)
+ ".hdf5"
)
filename = filename.replace("+", "").replace("e0", "e")
filename = "".join(filename.split())
F = h5py.File(filename, "w")
F.create_group("PartType0")
F.create_group("Header")
F["Header"].attrs["NumPart_ThisFile"] = [
N_gas,
0,
0,
0,
0,
(1 if M_BH > 0 else 0),
]
F["Header"].attrs["NumPart_Total"] = [
N_gas,
0,
0,
0,
0,
(1 if M_BH > 0 else 0),
]
F["Header"].attrs["MassTable"] = [M_gas / N_gas, 0, 0, 0, 0, M_BH]
F["Header"].attrs["BoxSize"] = boxsize
F["Header"].attrs["Time"] = 0.0
F["PartType0"].create_dataset("Masses", data=mgas[ind])
F["PartType0"].create_dataset("Coordinates", data=x[ind, :])
F["PartType0"].create_dataset("Velocities", data=v[ind, :])
F["PartType0"].create_dataset("ParticleIDs", data=np.arange(N_gas) + 1)
F["PartType0"].create_dataset("InternalEnergy", data=u[ind])
F["PartType0"].create_dataset("Density", data=rho[ind])
F["PartType0"].create_dataset("SmoothingLength", data=h[ind])
if M_BH > 0:
F.create_group("PartType5")
F["PartType5"].create_dataset("Masses", data=np.array([M_BH]))
F["PartType5"].create_dataset("BH_Mass", data=np.array([M_BH]))
F["PartType5"].create_dataset("Coordinates", data=center)
F["PartType5"].create_dataset("Velocities", data=v[0, :] * 0.0)
F["PartType5"].create_dataset("ParticleIDs", data=np.array([N_gas + 1]))
F["PartType5"].create_dataset("SinkRadius", data=np.array([Rsink]))
F.close()
if GMC_units:
delta_m = M_gas / N_gas
rhocrit = 421 / delta_m**2
rho_avg = 3 * M_gas / (R**3) / (4 * np.pi)
softening = 0.000173148 # 100AU/2.8 #(delta_m/rhocrit)**(1./3)
ncrit = 1.0e11 # 8920 / delta_m**2
tff = 8.275e-3 * rho_avg**-0.5
mdot_Bondi = (
np.exp(1.5) * np.pi * (G**2) * (M_BH**2) * rho_gas / (csound**3)
)
tend_Bondi = 2.0 * (2.0 * G * M_BH / (csound**3))
print(
"Bondi accretion parameters: \n \t Mgas:\t\t",
M_gas,
"\n \t Mdot:\t\t",
mdot_Bondi,
"\n \t Rsonic:\t",
rsonic_Bondi,
"\n \t Rsink:\t\t",
Rsink,
"\n \t t_end:\t\t",
tend_Bondi,
"\n \t m_acc:\t\t",
tend_Bondi * mdot_Bondi,
"\n \t f_acc:\t\t",
tend_Bondi * mdot_Bondi,
)
paramsfile = str(
open(
os.path.realpath(__file__).replace(
"MakeCloud_Bondi.py", "params.txt"
),
"r",
).read()
)
replacements = {
"NAME": "../ICs/" + filename.replace(".hdf5", ""),
"DTSNAP": tend_Bondi / 200,
"SOFTENING": softening,
"GASSOFT": 2.0e-8,
"TMAX": tend_Bondi,
"RHOMAX": ncrit,
"BOXSIZE": boxsize,
"OUTFOLDER": "output_%g" % (Rs_over_Rsonic),
}
print(replacements["NAME"])
# print(paramsfile)
for k in replacements.keys():
paramsfile = paramsfile.replace(k, str(replacements[k]))
open("params_" + filename.replace(".hdf5", "") + ".txt", "w").write(
paramsfile
)