{
  "scope": "Audit of interface equilibria, infrared coefficient and conditional physical scales",
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      "table_force_absolute_error": 1.1349744452647872e-08
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  ],
  "physical_scale_comparison": {
    "L8_over_lattice_spacing": 0.5069893620198437,
    "a0_m_s2": 2.2259991340534955e-10,
    "solar_nominal_GM_m3_s2": 1.3271244e+20,
    "solar_MOND_radius_m": 772135146692500.1,
    "one_copy_confinement_lattice_bound_m": 0.00019815110976763734,
    "one_copy_confinement_L8_bound_m": 0.00010046050472461847,
    "conditional_L8_over_solar_MOND_radius": 1.30107410801009e-19,
    "conditional_copies_to_set_L8_equal_solar_MOND_radius": 3.4897302884587118e+75,
    "assumptions": [
      "c_D=c",
      "Physical layers satisfy Sigma*thickness <= 1",
      "Confinement thickness >= v0*a_lattice/Omega",
      "The copy-count example retains the same critical matching"
    ],
    "interpretation": "A dimensional scale comparison, not a bound on the nonlinear solar quadrupole",
    "constants_sources": [
      "https://physics.nist.gov/cuu/Constants/Table/allascii.txt",
      "https://arxiv.org/abs/1510.07674"
    ]
  },
  "checks": {
    "maximum_stationarity_residual": 9.613017476684917e-10,
    "minimum_constrained_curvature": 0.03305779852859182,
    "maximum_profile_refinement_relative": 4.473861057207824e-06,
    "additional_filling_momenta": 392
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  "source_sha256": "ec74fa45693a9676a7d0416f87b2fe8b2c294f8de7f03f1b79ad0fba919096c5",
  "input_sha256": {
    "outputs/dark_equilibrium/summary.json": "dbdf0e1a69417cc578dbf80eed5daa22fceb0ce09d5514a42bce03e144fa76da",
    "outputs/dark_spatial_ir_summary.json": "85cc887850cdae0a5c2ad9202658ec8e0b444e6bd0b37a485201215358e86e79",
    "outputs/dark_scale_summary.json": "7eaee6f62ecec1c3917511051489c550f76031620a08d56872d137b3ddc094f6"
  }
}