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166 lines
4.6 KiB
Python
166 lines
4.6 KiB
Python
#!/usr/bin/env python
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"""
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Integrator
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Integrate differential equations.
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@ Author: Moussouni, Yaël (MSc student) & Bhat, Junaid Ramzan (MSc student)
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@ Institution: Université de Strasbourg, CNRS, Observatoire astronomique
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de Strasbourg, UMR 7550, F-67000 Strasbourg, France
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@ Date: 2025-01-01
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Licence:
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Order and Chaos in a 2D potential
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Copyright (C) 2025 Yaël Moussouni (yael.moussouni@etu.unistra.fr)
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Bhat, Junaid Ramzan (junaid-ramzan.bhat@etu.unistra.fr)
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integrator.py
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Copyright (C) 2025 Yaël Moussouni (yael.moussouni@etu.unistra.fr)
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Bhat, Junaid Ramzan (junaid-ramzan.bhat@etu.unistra.fr)
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This program is free software: you can redistribute it and/or modify
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it under the terms of the GNU General Public License as published by
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the Free Software Foundation; either version 3 of the License, or
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(at your option) any later version.
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This program is distributed in the hope that it will be useful,
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but WITHOUT ANY WARRANTY; without even the implied warranty of
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MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
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GNU General Public License for more details.
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You should have received a copy of the GNU General Public License
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along with this program. If not, see https://www.gnu.org/licenses/.
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"""
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import numpy as np
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def euler(t0: float,
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W0: np.ndarray,
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h: float,
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n: int,
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func):
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"""Euler method adapted for state vector [[x, y], [u, v]]
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@ params
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- t0: initial time value
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- W0: initial state vector [[x, y], [u, v]]
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- h: step size (time step)
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- n: number of steps
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- func: RHS of differential equation
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@returns:
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- t, W: time and state (solution) arrays
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"""
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time = np.zeros(n)
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W = np.zeros((n,) + np.shape(W0))
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t = t0
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w = W0
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for i in range(n):
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k1 = func(t, w)
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w = w + h*k1
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t = t + h
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time[i] = t
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W[i] = w
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return time, W
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def rk2(t0: float,
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W0: np.ndarray,
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h: float,
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n: int,
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func):
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"""RK2 method adapted for state vector [[x, y], [u, v]]
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@ params
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- t0: initial time value
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- W0: initial state vector [[x, y], [u, v]]
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- h: step size (time step)
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- n: number of steps
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- func: RHS of differential equation
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@returns:
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- t, W: time and state (solution) arrays
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"""
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time = np.zeros(n)
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W = np.zeros((n,) + np.shape(W0))
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t = t0
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w = W0
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for i in range(n):
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k1 = func(t, w)
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k2 = func(t + h/2, w + h/2*k1)
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w = w + h*k2
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t = t + h
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time[i] = t
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W[i] = w
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return time, W
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def rk4(t0: float,
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W0: np.ndarray,
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h: float,
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n: int,
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func):
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"""RK4 method adapted for state vector [[x, y], [u, v]]
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@ params
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- t0: initial time
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- W0: initial state vector [[x, y], [u, v]]
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- h: step size (time step)
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- n: number of steps
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- func: RHS of differential equation
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@returns:
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- t, W: time and state (solution) arrays
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"""
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time = np.zeros(n)
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W = np.zeros((n,) + np.shape(W0))
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# to accommodate the state vector
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t = t0
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w = W0
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for i in range(n):
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k1 = func(t, w)
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k2 = func(t + h/2, w + h/2*k1)
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k3 = func(t + h/2, w + h/2*k2)
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k4 = func(t + h, w + h*k3)
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w = w + h*(k1/6 + k2/3 + k3/3 + k4/6)
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t = t + h
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time[i] = t
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W[i] = w
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return time, W
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def integrator_type(t0, W0, h, n, func, integrator):
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return integrator(t0, W0, h, n, func)
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def kepler_analytical(t0: float,
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W0: np.ndarray,
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h: float,
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n: int):
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"""Computes the evolution from the Kepler potential derivative
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@ params
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- t0: initial time value
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- W0: initial state vector [[x, y], [u, v]]
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- h: step size (time step)
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- n: number of steps
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@returns:
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- t, W: time and state (solution) arrays
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"""
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X0 = W0[0 ,0]
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Y0 = W0[0, 1]
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U0 = W0[1, 0]
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V0 = W0[1, 1]
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time = np.arange(t0, t0 + n*h, h)
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W = np.zeros((n,) + np.shape(W0))
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R0 = np.sqrt(X0**2 + Y0**2)
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Omega0 = np.sqrt(U0**2 + V0**2)/R0
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X = R0 * np.cos(Omega0 * time)
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Y = R0 * np.sin(Omega0 * time)
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U = -R0 * Omega0 * np.sin(Omega0 * time)
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V = R0 * Omega0 * np.cos(Omega0 * time)
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W = np.array([[X, Y], [U, V]])
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W = np.swapaxes(W, 0, 2)
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W = np.swapaxes(W, 1, 2)
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return time, W
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