{
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  "decimal_precision_digits": 150,
  "quadrature": "Independent 48- and 96-point Gauss-Legendre nodes, computed in Decimal arithmetic.",
  "scope": "Conditional asymptotic consistency of the printed finite-eta scalar forces; no full MHD, corrected EOS evolution, source-code execution or figure reproduction.",
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  ],
  "maximum_48_vs_96_relative_quadrature_difference": "7.99238071439095032525411448978065261961884322717100401360101e-75",
  "source_locators": {
    "journal_doi": "10.1017/S0022377825100949",
    "cumulative_integral": "Eq.(2.29), p.7; printed ODE Eq.(2.31), p.7",
    "weak_and_strong_asymptotics": "Eqs.(3.2)\u2013(3.12), pp.11\u201313; Fig.4, p.14",
    "proposed_equal_order_threshold": "Eq.(3.13), p.15",
    "leading_coefficient": "Appendix B, Eqs.(B11)\u2013(B14), p.23"
  },
  "limits": [
    "A finite-window cooling-dominated regime is not ruled out at a fixed large coefficient.",
    "The limiting argument requires eta_c>0; simultaneous two-axis collapse is outside its assumptions.",
    "The 8/9 correction is generic only when the net limiting thermal coefficient is nonzero; cancellations and energy constants change subleading behavior.",
    "The source pressure formula independently fails its primitive EOS; this check does not substitute a claimed solution of corrected physical equations.",
    "No physical universal asymptotic exponent, astrophysical transition or actual Figure4 fit has been measured."
  ],
  "new_MHD_or_PIC_simulations": 0
}