File:Wigner quasiprobability distribution of superpositioned Fock states.webm

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Original file (WebM audio/video file, VP9, length 7.5 s, 2,400 × 1,600 pixels, 506 kbps overall, file size: 464 KB)

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English: Wigner quasiprobability distribution of superpositioned Fock states, for .

Matplotlib code

import matplotlib.pyplot as plt
import matplotlib as mpl
import numpy as np
from IPython.display import display
from qutip import (about, basis, coherent, coherent_dm, displace, fock, ket2dm,
                   plot_wigner, squeeze, thermal_dm, wigner_cmap, wigner)

import scipy.ndimage
import os
from tqdm import tqdm

def rotate_and_crop(array, angle, xvec, yvec):
    rotated_array = scipy.ndimage.rotate(array, -angle, reshape=False)
    rows, cols = rotated_array.shape
    center_row, center_col = rows // 2, cols // 2
    target_rows, target_cols = len(yvec), len(xvec)
    start_row = center_row - target_rows // 2
    end_row = start_row + target_rows
    start_col = center_col - target_cols // 2
    end_col = start_col + target_cols
    return rotated_array[start_row:end_row, start_col:end_col]

def plot_wigner_marginals(W, xvec, yvec, marginal_max, resolution=200, angle=0):
    wmap = wigner_cmap(W)
    wlim = np.abs(W).max()
    cmap = plt.colormaps['RdBu']

    fig = plt.figure()
    n, m = 5, 1
    fig, axes = plt.subplot_mosaic(
        [ ["top"] * n + ["3d"] * m ] * m + [ ["mid"] * n + ["right"] * m] * n,
    figsize=(20, 20),
    layout="constrained",
    width_ratios=[1.05] * (n+m))

    ax = axes["mid"]
    norm = mpl.colors.Normalize(-wlim, wlim)
    ax.contourf(xvec, yvec, W, resolution // 3, norm=norm, cmap=cmap)
    

    ax = axes["top"]
    x_marginal = np.sum(W, axis=0)
    y_marginal = np.sum(W, axis=1)
    ax.fill_between(xvec, x_marginal, 0, color='#938fba', alpha=0.5)
    ax.plot(xvec, x_marginal, color='#4a5a90')
    ax.set_xlim(min(xvec), max(xvec))
    ax.set_ylim(0, marginal_max * 1.05)
    ax.set_xticks([])
    ax.set_yticks([])

    ax = axes["right"]
    ax.fill_betweenx(yvec, np.sum(W, axis=1), 0, color='#938fba', alpha=0.5)
    ax.plot(y_marginal, yvec, color='#4a5a90')
    ax.set_xlim(0, marginal_max * 1.05)
    ax.set_ylim(min(yvec), max(yvec))
    ax.set_xticks([])
    ax.set_yticks([])

    ax = axes["3d"]
    ax.axis('off')

    return fig

def plot_wigner_with_marginals(psi, **kwargs):
    
    radius = kwargs.get('radius', 5) 
    resolution = kwargs.get('resolution', 500)
    angles = kwargs.get('angles', np.linspace(0, 2*np.pi, 100))
    dir_path = kwargs.get('dir_path', './output')
    
    xvec_upscaled = np.linspace(-radius*1.5, radius*1.5, int(resolution*1.5))
    yvec_upscaled = np.linspace(-radius*1.5, radius*1.5, int(resolution*1.5))
    xvec = np.linspace(-radius, radius, int(resolution))
    yvec = np.linspace(-radius, radius, int(resolution))

    W_upscaled = wigner(psi, xvec_upscaled, yvec_upscaled)
    marginal_max = max(max(np.sum(W_upscaled, axis=0)), max(np.sum(W_upscaled, axis=1)))
    print(f"outputting to {dir_path}")
    for N, angle in tqdm(enumerate(angles)):
        W = rotate_and_crop(W_upscaled, angle, xvec, yvec)
        fig = plot_wigner_marginals(W, xvec, yvec, marginal_max=marginal_max, resolution=resolution, angle=angle)

        if not os.path.exists(dir_path):
            os.makedirs(dir_path)
        fig.savefig(f"{dir_path}/{N:03d}.png",bbox_inches='tight')
        plt.close(fig)
    
mpl.use('agg')

configs = {
    "N_dim" : 40,
    "radius" : 3.5,
    "resolution" : 500,
    "angles" : [i * 2 for i in range(180)],
    "dir_path" : ""
}

for n1, n2 in [(0, 0), (0, 1), (0, 2), (1, 1), (1, 2), (2, 2)]:
    psi = (fock(configs["N_dim"], n1) + fock(configs["N_dim"], n2)).unit()
    configs["dir_path"] = f"./fock/fock_{n1}_{n2}"
    plot_wigner_with_marginals(psi, **configs)



Sh code

for dir in ./*/; do
    # Extract folder name
    folder_name=$(basename "$dir")
    # Create output path
    output_path="./${folder_name}.webm"
    # Convert images to webm
    echo $output_path
    ffmpeg -y -framerate 24 -i "$dir"%03d.png -c:v libvpx-vp9 -b:v 0 -crf 30 -pix_fmt yuva420p "$output_path"
done

ffmpeg -y \
  -i ./fock_0_0.webm \
  -i ./fock_0_1.webm \
  -i ./fock_0_2.webm \
  -i ./fock_1_1.webm \
  -i ./fock_1_2.webm \
  -i ./fock_2_2.webm \
  -filter_complex "
    [0:v]scale=800:800[v0];
    [1:v]scale=800:800[v1];
    [2:v]scale=800:800[v2];
    [3:v]scale=800:800[v3];
    [4:v]scale=800:800[v4];
    [5:v]scale=800:800[v5];
    [v0][v1][v2]hstack=inputs=3[row0];
    [v3][v4][v5]hstack=inputs=3[row1];
    [row0][row1]vstack=inputs=2[out]
  " \
  -map "[out]" \
   -c:v libvpx-vp9 -b:v 0 -crf 30 -pix_fmt yuva420p \
  output_grid.webm

Date
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Author Cosmia Nebula

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Date/TimeThumbnailDimensionsUserComment
current03:58, 31 August 20247.5 s, 2,400 × 1,600 (464 KB)Cosmia Nebula (talk | contribs)Uploaded while editing "Wigner quasiprobability distribution" on en.wikipedia.org

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