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MSc2-Project-Chaos/Source/integrator.py
Yael-II 61a5a5e50f update
2025-01-22 00:00:33 +01:00

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Python

#!/usr/bin/env python
"""
Integrator
Integrate differential equations.
@ 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)
integrator.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
def euler(t0: float,
W0: np.ndarray,
h: float,
n: int,
func):
"""Euler method adapted for state vector [[x, y], [u, v]]
@ params
- t0: initial time value
- W0: initial state vector [[x, y], [u, v]]
- h: step size (time step)
- n: number of steps
- func: RHS of differential equation
@returns:
- t, W: time and state (solution) arrays
"""
time = np.zeros(n)
W = np.zeros((n,) + np.shape(W0))
t = t0
w = W0
for i in range(n):
k1 = func(t, w)
w = w + h*k1
t = t + h
time[i] = t
W[i] = w
return time, W
def rk2(t0: float,
W0: np.ndarray,
h: float,
n: int,
func):
"""RK2 method adapted for state vector [[x, y], [u, v]]
@ params
- t0: initial time value
- W0: initial state vector [[x, y], [u, v]]
- h: step size (time step)
- n: number of steps
- func: RHS of differential equation
@returns:
- t, W: time and state (solution) arrays
"""
time = np.zeros(n)
W = np.zeros((n,) + np.shape(W0))
t = t0
w = W0
for i in range(n):
k1 = func(t, w)
k2 = func(t + h/2, w + h/2*k1)
w = w + h*k2
t = t + h
time[i] = t
W[i] = w
return time, W
def rk4(t0: float,
W0: np.ndarray,
h: float,
n: int,
func):
"""RK4 method adapted for state vector [[x, y], [u, v]]
@ params
- t0: initial time
- W0: initial state vector [[x, y], [u, v]]
- h: step size (time step)
- n: number of steps
- func: RHS of differential equation
@returns:
- t, W: time and state (solution) arrays
"""
time = np.zeros(n)
W = np.zeros((n,) + np.shape(W0))
# to accommodate the state vector
t = t0
w = W0
for i in range(n):
k1 = func(t, w)
k2 = func(t + h/2, w + h/2*k1)
k3 = func(t + h/2, w + h/2*k2)
k4 = func(t + h, w + h*k3)
w = w + h*(k1/6 + k2/3 + k3/3 + k4/6)
t = t + h
time[i] = t
W[i] = w
return time, W
def integrator_type(t0, W0, h, n, func, integrator):
return integrator(t0, W0, h, n, func)
def kepler_analytical(t0: float,
W0: np.ndarray,
h: float,
n: int):
"""Computes the evolution from the Kepler potential derivative
@ params
- t0: initial time value
- W0: initial state vector [[x, y], [u, v]]
- h: step size (time step)
- n: number of steps
@returns:
- t, W: time and state (solution) arrays
"""
X0 = W0[0 ,0]
Y0 = W0[0, 1]
U0 = W0[1, 0]
V0 = W0[1, 1]
time = np.arange(t0, t0 + n*h, h)
W = np.zeros((n,) + np.shape(W0))
R0 = np.sqrt(X0**2 + Y0**2)
Omega0 = np.sqrt(U0**2 + V0**2)/R0
X = R0 * np.cos(Omega0 * time)
Y = R0 * np.sin(Omega0 * time)
U = -R0 * Omega0 * np.sin(Omega0 * time)
V = R0 * Omega0 * np.cos(Omega0 * time)
W = np.array([[X, Y], [U, V]])
W = np.swapaxes(W, 0, 2)
W = np.swapaxes(W, 1, 2)
return time, W