{
  "visual_id": "A10",
  "title": "A finite inflationary history need not equilibrate",
  "classification": "new_simulation",
  "status": "validated_within_scope",
  "run_ids": [
    "20260927T155438746257Z-E21-stochastic"
  ],
  "experiment_ids": [
    "E21-stochastic"
  ],
  "claim_ids": [
    "C05",
    "C08"
  ],
  "input_files": [
    {
      "path": "runs/20260927T155438746257Z-E21-stochastic/probability-histories.npz",
      "sha256": "9fc27fb81c96c50045aae4661f5d8c29633c0602b6b5579b0175ad69dd54c489"
    },
    {
      "path": "runs/20260927T155438746257Z-E21-stochastic/finite-inflation.csv",
      "sha256": "2c9fe2689387b5987270b5c5f1c689359179167819c08018512fcbad050594c0"
    }
  ],
  "frame_data": "A10-frames.json",
  "frame_sha256": "f06c317e8c91f4d5a0490d33581f82f26b96053d22eb04c0223ce0405fcbb950",
  "caption": "Positive, conservative Fokker\u2013Planck evolution for a specified light spectator at fixed H, compared with the stationary distribution. Explicit initial conditions remain important. Only five saved times are played, with their unequal e-fold spacing labeled. This does not derive reheating, late domains or a cosmological measure.",
  "alt_text": "Probability curves starting in opposite minima retain different weights over a finite duration. A central initial state spreads into both wells, and all are compared with the stationary reference.",
  "time_interpolation": "Frames sample saved arrays or explicit analytic equations. Plot-line interpolation does not add a new evolution solve.",
  "generator_sha256": "3ab3602467624926777d30a93a98b83730c4c7c9094af6fb744ac01c4c92536c",
  "playback": "Paused by default, manual play and frame slider; motion stops when hidden or reduced-motion preference changes.",
  "extension_generator_sha256": "4dea479215b06587d2f9e396874350b65f06d7478fe9f631859a2bb1c30c5c80",
  "render_command": "uv run --offline --frozen python run.py full animations",
  "output_sha256": {
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    "-transcript.md": "7d7c5bd83a35445a0182dc45c9d8ba58070db55190c4ca27d2febe0b7eba0481"
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}