{
  "title": "Large N and Semiclassical Bulk Criteria: structure map",
  "chapter": "Large N and Semiclassical Bulk Criteria",
  "kind": "structure",
  "schematic": true,
  "not_to_scale": true,
  "stages": [
    "normalized large-N data",
    "factorization and spectrum",
    "gap and coupling hierarchy",
    "locality and correction tests",
    "semiclassical-bulk criterion"
  ],
  "claims": [
    {
      "object": "factorization",
      "required_declaration": "operator normalization and N scaling",
      "diagnostic": "connected-correlator hierarchy",
      "licensed_conclusion": "classical large-N organization",
      "unsupported_promotion": "geometric locality"
    },
    {
      "object": "large gap",
      "required_declaration": "single-trace sector and gap definition",
      "diagnostic": "Regge and finite-gap tests",
      "licensed_conclusion": "heavy higher-spin sector",
      "unsupported_promotion": "a sufficient local bulk"
    },
    {
      "object": "finite-N sector",
      "required_declaration": "order of N, time, and energy limits",
      "diagnostic": "exponential and recurrence checks",
      "licensed_conclusion": "a stated asymptotic approximation",
      "unsupported_promotion": "exact late-time behavior"
    }
  ],
  "takeaway": "Factorization, sparsity, a higher-spin gap, and controlled corrections are independent criteria; large N alone does not imply Einstein gravity."
}