{
  "id": "MAP-01",
  "uri": "https://cosmological-constant.org/claims/#MAP-01",
  "record_type": "Scientific claim",
  "status": "Proposed",
  "dependencies": [
    "NUM-01",
    "GS-02"
  ],
  "downstream_claims": [
    "OBS-02"
  ],
  "technical_statement": "Given the proposed global four-form action and its derived field equation <R> = 4 M_P^2 q_WZ, the compact charge is identified with the residual curvature on a maximally symmetric vacuum: Lambda/M_P^2 = q_WZ.",
  "public_statement": "The proposed gravity-side completion identifies the calculated compact response with the residual curvature of empty space. This identification is a separate step from the compact calculation and carries the completion’s Proposed status.",
  "qualifier": "Distinct from NUM-01, which computes q_WZ within the compact channel; the identification inherits the global-source action and its source-charge normalisation. The late-time branch (GS-03) enters at the observational comparison (OBS-02).",
  "source_in_paper": "CC Paper I v1.0, Theorem 6 and Appendix E",
  "external_foundations": "HenneauxTeitelboim1989; KaloperPadilla2014; KaloperPadillaStefanyszynZahariade2016",
  "limits_open_issues": "The identification stands or falls with the proposed completion; a completion returning a different action-level normalisation changes the predicted curvature.",
  "relations": "",
  "version_history": "v1.4 (2026-08-03): added on internal review; separates the global identification from the compact calculation NUM-01.; v1.6 (2026-08-08): GS-03 moved downstream to OBS-02: the proposed action alone gives the maximally symmetric vacuum relation; the trace-average branch enters at the late-time observational identification",
  "register_version": "v1.6"
}