{
  "scope": "Critical spatial susceptibility of the full eight-band LQ8 Hamiltonian; no solar field solution",
  "predicted_coefficient": 0.12437964877624864,
  "reflection_control_error": 4.547473508864641e-13,
  "quadratures": {
    "coarse": [
      16,
      24
    ],
    "fine": [
      24,
      40
    ]
  },
  "results": [
    {
      "Q": 0.1,
      "coarse_delta_kernel": 0.014204490690160002,
      "fine_delta_kernel": 0.014204494363910195,
      "coefficient": 0.14204494363910194,
      "relative_error_to_IR_coefficient": 0.1420272129456812,
      "relative_quadrature_change": 2.5863294382932404e-07
    },
    {
      "Q": 0.03,
      "coarse_delta_kernel": 0.003890509189897204,
      "fine_delta_kernel": 0.00389051028591763,
      "coefficient": 0.12968367619725435,
      "relative_error_to_IR_coefficient": 0.04264385269769755,
      "relative_quadrature_change": 2.817163676086121e-07
    },
    {
      "Q": 0.01,
      "coarse_delta_kernel": 0.0012614759625341884,
      "fine_delta_kernel": 0.0012614763276946662,
      "coefficient": 0.1261476327694666,
      "relative_error_to_IR_coefficient": 0.01421441538557855,
      "relative_quadrature_change": 2.894707334521459e-07
    },
    {
      "Q": 0.003,
      "coarse_delta_kernel": 0.00037472995404448054,
      "fine_delta_kernel": 0.00037473006358592346,
      "coefficient": 0.12491002119530782,
      "relative_error_to_IR_coefficient": 0.004264141475534,
      "relative_quadrature_change": 2.9232093595910564e-07
    },
    {
      "Q": 0.001,
      "coarse_delta_kernel": 0.00012455639464316676,
      "fine_delta_kernel": 0.00012455643115788568,
      "coefficient": 0.12455643115788569,
      "relative_error_to_IR_coefficient": 0.0014213127579663087,
      "relative_quadrature_change": 2.9315803759944997e-07
    },
    {
      "Q": 0.0003,
      "coarse_delta_kernel": 3.732979199364305e-05,
      "fine_delta_kernel": 3.7329802947982674e-05,
      "coefficient": 0.12443267649327559,
      "relative_error_to_IR_coefficient": 0.000426337568474322,
      "relative_quadrature_change": 2.934475608422842e-07
    },
    {
      "Q": 0.0001,
      "coarse_delta_kernel": 1.2439728169189932e-05,
      "fine_delta_kernel": 1.243973182062012e-05,
      "coefficient": 0.1243973182062012,
      "relative_error_to_IR_coefficient": 0.00014206045865550188,
      "relative_quadrature_change": 2.935296548995427e-07
    }
  ],
  "source_sha256": "a0cdd3e853ca62bb0d1feea6abeb6b603fdb336e647674d74c5bd2039b7a8c02",
  "dependencies_sha256": {
    "dark_band_probe.py": "d7ce52e95d0b0677abbd342ef3bd28367afbe8b63bd70c68178f5d4c9be687fd",
    "dark_profile_probe.py": "4283add4748dc5b145c0a55cd3da1458ed64a58aa196172c248b03f32cde628d",
    "dark_response_report.py": "0a5fb30270ee2f79cf78d80452d293474689025f71fdd77f177844a165946039"
  },
  "limitations": [
    "The background is uniform and critical, with infinitesimal source perturbations",
    "The physical lattice spacing is not determined",
    "An infrared response coefficient is not the full nonlocal gravitational equation"
  ]
}