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MSc2-Project-Chaos/Source/gottwald_melbourne.py
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#!/usr/bin/env python
"""
Gottwald and Melbourne method
Study chaotic behaviour with the method of Gottwald & Melbourne (2003).
@ Author: Moussouni, Yaël (MSc student) & Bhat, Junaid Ramzan (MSc student)
@ Institution: Université de Strasbourg, CNRS, Observatoire astronomique
de Strasbourg, UMR 7550, F-67000 Strasbourg, France
@ Date: 2025-01-01
Licence:
Order and Chaos in a 2D potential
Copyright (C) 2025 Yaël Moussouni (yael.moussouni@etu.unistra.fr)
Bhat, Junaid Ramzan (junaid-ramzan.bhat@etu.unistra.fr)
gottwald_melbourne.py
Copyright (C) 2025 Bhat, Junaid Ramzan (junaid-ramzan.bhat@etu.unistra.fr)
This program is free software: you can redistribute it and/or modify
it under the terms of the GNU General Public License as published by
the Free Software Foundation; either version 3 of the License, or
(at your option) any later version.
This program is distributed in the hope that it will be useful,
but WITHOUT ANY WARRANTY; without even the implied warranty of
MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
GNU General Public License for more details.
You should have received a copy of the GNU General Public License
along with this program. If not, see https://www.gnu.org/licenses/.
"""
import numpy as np
import matplotlib.pyplot as plt
from scipy.integrate import cumulative_trapezoid
import potentials as pot
import integrator as itg
import initial_conditions as init
# -----------------------------------------------------------------------------------
# Parameters
# -----------------------------------------------------------------------------------
DEFAULT_N_iter = 30000
DEFAULT_h = 0.01
DEFAULT_c = 1.7
E_all = np.array([1/100, 1/12, 1/10, 1/8, 1/6])
if "YII_1" in plt.style.available: plt.style.use("YII_1")
# -----------------------------------------------------------------------------------
# 1) Integrate HénonHeiles and Return x(t), etc.
# -----------------------------------------------------------------------------------
def compute_coordinates(E: float,
N_iter: int = DEFAULT_N_iter,
h: float = DEFAULT_h,
N_part: int = 1) -> tuple:
"""
Integrate HénonHeiles for N_iter steps at step size h for a single
random initial condition at energy E.
Returns:
t_part: array of times of length N_iter
x_part, y_part, u_part, v_part: arrays of length N_iter each
"""
# Generate 1 initial condition at energy E
W_init = init.n_energy_part(pot.hh_potential, N_part, E)
W0 = W_init[:, :, 0] # take first particle
# Perform integration using RK4
final_t, sol_array = itg.rk4(0.0, W0, h, N_iter, pot.hh_evolution)
# Reconstruct the time array using step size and number of iterations
# Extract coordinate arrays
x_part = sol_array[:, 0, 0]
y_part = sol_array[:, 0, 1]
u_part = sol_array[:, 1, 0]
v_part = sol_array[:, 1, 1]
return final_t, x_part, y_part, u_part, v_part
# -----------------------------------------------------------------------------------
# 2) Compute theta(t_i) in discrete form
# -----------------------------------------------------------------------------------
def compute_theta_discrete(t_array, x_array, c=DEFAULT_c):
int_x = cumulative_trapezoid(x_array, t_array, initial=0.0)
theta_array = c * t_array + int_x
return theta_array
# -----------------------------------------------------------------------------------
# 3) Compute p(t_i) in discrete form
# -----------------------------------------------------------------------------------
def compute_p_discrete(t_array, x_array, theta_array):
integrand = x_array * np.cos(theta_array)
p_array = cumulative_trapezoid(integrand, t_array, initial=0.0)
return p_array
# -----------------------------------------------------------------------------------
# Main: Compute p(t) for each energy and plot on a single graph
# -----------------------------------------------------------------------------------
if __name__ == "__main__":
fig, ax = plt.subplots() # single figure and axis
# Loop over energies and plot each p(t) on the same axis
i = 0
line_styles = ["-", "-", "--", ":", ":"]
for E in E_all:
# 1) Integrate HénonHeiles for current energy
t_part, x_part, y_part, u_part, v_part = compute_coordinates(E)
# 2) Compute theta(t) for current energy
theta_arr = compute_theta_discrete(t_part, x_part, c=DEFAULT_c)
# 3) Compute p(t) for current energy
p_arr = compute_p_discrete(t_part, x_part, theta_arr)
# Plot p(t) for the current energy on the same axis
ax.plot(t_part, p_arr,
line_styles[i],
color="C{}".format(i).replace("C1", "C5"),
label="$E={:.3f}$".format(E))
i += 1
#ax.set_title("$p(t)$ (MelbourneGottwald Test)")
ax.set_xlabel("$t$")
ax.set_ylabel("$p(t)$")
ax.legend()
# Enable both major and minor gridlines
#ax.grid(which='both', linestyle='--', linewidth=0.5)
#ax.minorticks_on()
fig.tight_layout()
fig.savefig("Figs/gottwald_melbourne.pdf")
plt.show()