Created
September 8, 2012 23:22
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Python script which solves for the gravitational potential of a spherically symmetric star with a Lane-Emden polytrope density profile
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import numpy as np | |
import matplotlib.pyplot as plt | |
def density(r): | |
if density.outside: | |
return 0.0 | |
else: | |
z = density.rho_c * np.sin(r/R) / (r/R) if r > 1e-8 else 0.0 | |
if z < 0.0: | |
density.outside = True | |
return 0.0 | |
return z | |
def f(y, r): | |
psi, phi = y[0], y[1] | |
psi_p = 4*np.pi*G*density(r) - (2 * psi/r if r > 1e-8 else 0.0) | |
phi_p = psi | |
return np.array([psi_p, phi_p]) | |
G = 0.1 # Gravitational constant | |
R = 1.0 # Characteristic radius | |
psi = [ ] | |
phi = [ ] | |
rad = [ ] | |
rho = [ ] | |
dr = 1e-3 | |
r = 0.0 | |
y = np.array([0.0, 0.0]) | |
density.outside = False | |
density.rho_c = 1.0 | |
while r < 10 * R: | |
k1 = f(y, r) | |
k2 = f(y + 0.5*k1*dr, r + 0.5*dr) | |
k3 = f(y + 0.5*k2*dr, r + 0.5*dr) | |
k4 = f(y + 1.0*k3*dr, r + 1.0*dr) | |
y += (k1 + 2*k2 + 2*k3 + k4) * dr / 6.0 | |
r += dr | |
phi.append(y[1]) | |
rad.append(r) | |
rho.append(density(r)) | |
plt.plot(rad, phi, label=r"$\phi(r)$", ls='-.', lw=2) | |
plt.plot(rad, rho, label=r"$\rho(r)$", ls='--', lw=2) | |
plt.legend(loc='best') | |
plt.show() |
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