{
  "schema": "sandboxphysics.emri-frequency-evolution.inputs/1",
  "units": {
    "geometric": "G = c = 1, lengths and times in units of the large black hole mass M",
    "energyFlux": "dE/dt in units of (mu/M)^2, dimensionless in geometric units",
    "frequency": "hertz after multiplying times by M * G M_sun / c^3"
  },
  "fluxTable": {
    "source": "R. Fujita and H. Tagoshi, Prog. Theor. Phys. 112, 415 (2004), arXiv:gr-qc/0410018v1, Table VII",
    "caption": "The gravitational wave luminosity, up through l = 6, for various q and orbital radii r0/M (q is the spin a/M; negative q is an orbit against the spin).",
    "interpretation": "Read as energy flux to infinity per (mu/M)^2. The normalisation and the 'to infinity' reading are inferences checked against the quadrupole and Tagoshi-Sasaki post-Newtonian limits; the horizon flux is not included.",
    "transcribedRows": "r0/M = 6..20 only; transcribed by hand from the PDF and cross-checked against the sum of Table III at r0 = 6M",
    "spins": [
      -0.9,
      -0.6,
      -0.3,
      0.0,
      0.3,
      0.6,
      0.9
    ],
    "radii": [
      6,
      8,
      10,
      12,
      14,
      16,
      18,
      20
    ],
    "values": [
      [
        0.0020073,
        0.0015089,
        0.0011707,
        0.00093619,
        0.00077061,
        0.00065182,
        0.00056555
      ],
      [
        0.00029124,
        0.00025217,
        0.00022097,
        0.00019593,
        0.00017577,
        0.00015948,
        0.00014631
      ],
      [
        7.9272e-05,
        7.2377e-05,
        6.6505e-05,
        6.1499e-05,
        5.7229e-05,
        5.3588e-05,
        5.0488e-05
      ],
      [
        2.9095e-05,
        2.7287e-05,
        2.5693e-05,
        2.4289e-05,
        2.3052e-05,
        2.1965e-05,
        2.101e-05
      ],
      [
        1.2794e-05,
        1.219e-05,
        1.1646e-05,
        1.1157e-05,
        1.0717e-05,
        1.0323e-05,
        9.9699e-06
      ],
      [
        6.3614e-06,
        6.1235e-06,
        5.9062e-06,
        5.7079e-06,
        5.5272e-06,
        5.3627e-06,
        5.2134e-06
      ],
      [
        3.4599e-06,
        3.3541e-06,
        3.2565e-06,
        3.1666e-06,
        3.0837e-06,
        3.0075e-06,
        2.9376e-06
      ],
      [
        2.0155e-06,
        1.964e-06,
        1.916e-06,
        1.8714e-06,
        1.8301e-06,
        1.7918e-06,
        1.7563e-06
      ]
    ]
  },
  "constants": {
    "solarMassTimeSeconds": 4.925490947e-06,
    "julianYearSeconds": 31557600
  },
  "cases": [
    {
      "id": "schwarzschild-10-to-6",
      "spin": 0.0,
      "startRadius": 10,
      "stopRadius": 6.003,
      "massRatio": 1e-05,
      "blackHoleMassSolar": 1000000.0
    },
    {
      "id": "prograde-a0.9-10-to-6",
      "spin": 0.9,
      "startRadius": 10,
      "stopRadius": 6.0,
      "massRatio": 1e-05,
      "blackHoleMassSolar": 1000000.0
    },
    {
      "id": "retrograde-a-0.9-20-to-10",
      "spin": -0.9,
      "startRadius": 20,
      "stopRadius": 10.0,
      "massRatio": 1e-05,
      "blackHoleMassSolar": 1000000.0
    }
  ],
  "integration": {
    "method": "composite Simpson rule in ln r",
    "intervals": 2000
  }
}