![```python from tqdm import tqdm import numpy as np import matplotlib.pyplot as plt from scipy.integrate import solve_ivp import os escape_size = 2.0 # If a trajectory is this distance away from 0, we assume it has escaped and stop simulating it. max_mu = 0.22 mu_resolution = 120 mus = np.linspace(0.001, max_mu, mu_resolution) ** 2 for i, mu in enumerate(tqdm(mus)): fig, ax = plt.subplots(figsize=(16,16)) def system(t, y): v, w = y dv = mu * v + w - v**2 dw = -v + mu * w + 2 * v**2 dv *= (np.abs(v) < 2.0) * (np.abs(w) < 2.0) dw *= (np.abs(v) < 2.0) * (np.abs(w) < 2.0) return [dv, dw] def system_reversed(t, y): v, w = y dv = mu * v + w - v**2 dw = -v + mu * w + 2 * v**2 dv *= (np.abs(v) < 2.0) * (np.abs(w) < 2.0) dw *= (np.abs(v) < 2.0) * (np.abs(w) < 2.0) return [-dv, -dw] x_root = (mu**2+1)/(2+mu) y_root = -mu * x_root + x_root ** 2 vmin, vmax, wmin, wmax = -0.4,0.4,-0.4,0.4 # Hopf bifurcation circle if mu > 0: thetas = np.linspace(0, 2*np.pi, 1000) xs = np.sqrt(2*mu) * np.cos(thetas) ys = -np.sqrt(2*mu) * np.sin(thetas) ax.plot(xs, ys, color='r', linewidth=1, label="$\mu^{1/2}$ order") xs += mu * (2-2/3 * np.sin(2*thetas)-2/3 * np.cos(2*thetas)) ys += mu * (1+4/3*np.sin(2*thetas) - 1/3*np.cos(2*thetas)) ax.plot(xs, ys, color='b', linewidth=1, label="$\mu$ order") xs += mu**1.5 / np.sqrt(72) * (5 * np.sin(3*thetas) - np.cos(3*thetas)) ys += mu**1.5 / np.sqrt(72) * (36 * np.sin(thetas) + 28 * np.cos(thetas) - 5 * np.sin(3*thetas) + 7 * np.cos(3*thetas)) ax.plot(xs, ys, color='k', linewidth=1, label="$\mu^{3/2}$ order") radius = xs[0] t_span = np.array([0, 14]) trajectory_resolution = 10 epsilon = 0.01 initial_conditions = [] initial_conditions += [(x, 0) for x in np.linspace(vmin, vmax, trajectory_resolution)] initial_conditions_2 = [] if mu > 0: initial_conditions_2 = [(radius *(1 + dx), 0) for dx in np.linspace(-0.08, 0.08, 5)] sols = {} sols_2 = {} for ic in initial_conditions: sols[ic] = solve_ivp(system, [0,50], ic, dense_output=True, max_step=0.05) for ic in initial_conditions_2: sols_2[ic] = solve_ivp(system, [0, min(0.1 * t_span[1]/mu, 200)], ic, dense_output=True, max_step=0.05) vs = np.linspace(vmin, vmax, 200) v_axis = np.linspace(vmin, vmax, 20) w_axis = np.linspace(wmin, wmax, 20) v_values, w_values = np.meshgrid(v_axis, w_axis) dv, dw = system(0, [v_values, w_values]) # integral curves # ax.scatter([x for x, y in initial_conditions_2], [y for x, y in initial_conditions_2]) for ic in initial_conditions: sol = sols[ic] ax.plot(sol.y[0], sol.y[1],alpha=0.2, linewidth=0.5, color='k') for ic in initial_conditions_2: sol = sols_2[ic] ax.plot(sol.y[0], sol.y[1],alpha=0.3, linewidth=0.5, color='g') # vector fields arrow_lengths = np.sqrt(dv**2 + dw**2) alpha_values = 1 - (arrow_lengths / np.max(arrow_lengths))**0.4 ax.quiver(v_values, w_values, dv, dw, color='blue', linewidth=0.5, scale=25, alpha=alpha_values) ax.set_title(f'Hopf Bifurcation Model\n$\mu={mu:.4f](http://upload.wikimedia.org/wikipedia/commons/thumb/8/87/Hopf_bifurcation%2C_with_limit_cycle_up_to_order_3-2..gif/600px-Hopf_bifurcation%2C_with_limit_cycle_up_to_order_3-2..gif)
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|date=2023-04-26 |source=Own work |author=Cosmia Nebula }}
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