#!/usr/bin/env python """ Main: Compute Relative Area Computes the relative area covered bu the curves for different energies, to study ordered and chaotic regimes. @ 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) main_area.py Copyright (C) 2025 Yaël Moussouni (yael.moussouni@etu.unistra.fr) 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 from scipy.optimize import curve_fit import potentials as pot import energies as ene import integrator as itg import initial_conditions as init import poincare_sections as pcs OUT_DIR = "./Output/" FILENAME_PREFIX = "phase_separation_" EXTENSION = ".csv" DEFAULT_N_iter = int(1e5) DEFAULT_N_part = 200 DEFAULT_h = 0.005 E_all = np.linspace(1/100, 1/6, 20) def compute_mu(E: float, N_iter: int = DEFAULT_N_iter, N_part: int = DEFAULT_N_part, h: float = DEFAULT_h) -> tuple: """ Computes the phase-space squared distances for particles of given energy E. @params: - E: the total energy of each particles - N_iter: the number of iteration - N_part: the number of particles - h: integration steps @returns: - mu: phase-space squared distance """ W_1, W_2 = init.n_energy_2part(pot.hh_potential, N_part, E) t_1, positions_1 = itg.rk4(0, W_1, h, N_iter, pot.hh_evolution) x_1 = positions_1[:, 0, 0] y_1 = positions_1[:, 0, 1] u_1 = positions_1[:, 1, 0] v_1 = positions_1[:, 1, 1] t_2, positions_2 = itg.rk4(0, W_2, h, N_iter, pot.hh_evolution) x_2 = positions_2[:, 0, 0] y_2 = positions_2[:, 0, 1] u_2 = positions_2[:, 1, 0] v_2 = positions_2[:, 1, 1] dist_sq = (x_2[-25:] - x_1[-25:])**2 \ + (y_2[-25:] - y_1[-25:])**2 \ + (u_2[-25:] - u_1[-25:])**2 \ + (v_2[-25:] - v_1[-25:])**2 mu = np.sum(dist_sq, axis=0) return mu if __name__ == "__main__": mu_all = [] for i in range(len(E_all)): mu = compute_mu(E_all[i]) filename = OUT_DIR + FILENAME_PREFIX\ + str(i) + EXTENSION np.savetxt(filename, mu)