{
  "protocolVersion": "1.0",
  "name": "Omega Centauri Society Science Suite",
  "description": "MCP-accessible science suite for NGC 5139 (Omega Centauri): IMBH constraints, black-hole physics, Fermi Paradox analysis, SETI signal characterisation, Macro Transcension Hypothesis computation, and Kardashev-scale energy extraction. 23 client-side, zero-egress, single-file HTML calculators; each emits a OpenChainGraph-conformant artifact carrying a verifiable SHA-256 execution_hash (OpenChainGraph Standard v0.1).",
  "url": "https://mcp.omegacentauri.me/mcp",
  "preferredTransport": "JSONRPC",
  "version": "0.8.0",
  "provider": {
    "organization": "The Omega Centauri Society",
    "url": "https://omegacentauri.me"
  },
  "documentationUrl": "https://omegacentauri.me",
  "capabilities": {
    "streaming": false,
    "pushNotifications": false,
    "stateTransitionHistory": false,
    "extensions": [
      {
        "uri": "https://postoaklabs.github.io/chaingraph/ext/x-chaingraph/v0.1",
        "description": "Emits OpenChainGraph verifiable decision artifacts (hash-anchored). See the OpenChainGraph Standard v0.1.",
        "required": false,
        "params": {
          "spec_version": "0.8.0",
          "conformance_level": "L4",
          "graph_index": "https://omegacentauri.me/chaingraph.json",
          "internal_registry": "https://omegacentauri.me/tools/data/chaingraph.json",
          "verify_endpoint": "verify_execution_hash",
          "hash_alg": "sha256",
          "mandate_namespace": "me.omegacentauri",
          "tool_count": 34,
          "mandate_families": [
            "bh-physics",
            "fermi",
            "seti",
            "mth",
            "kardashev"
          ],
          "compliance_registers": [
            "peer-reviewed",
            "speculative",
            "model-dependent"
          ],
          "l2_runtime_chaining": true
        }
      }
    ]
  },
  "defaultInputModes": [
    "application/json",
    "text/plain"
  ],
  "defaultOutputModes": [
    "application/json",
    "text/plain"
  ],
  "skills": [
    {
      "id": "bh-physics",
      "name": "IMBH & Black-Hole Physics",
      "description": "Constrain and characterise a candidate intermediate-mass black hole in NGC 5139: stacked observational mass-window constraints, ADAF/SED accretion modelling, QPO mass-spin, shadow imaging, kinematics, dark-cluster alternatives, and astrometric forecasts. The Häberle 2024 lower bound (>=8,200 M-sun) and the competing upper limits are kept as distinct, irreconcilable bounds and are never collapsed to one number.",
      "tags": [
        "IMBH",
        "NGC 5139",
        "accretion",
        "kinematics",
        "pulsar-timing",
        "JWST"
      ],
      "examples": [
        "Compute the currently allowed IMBH mass window from the active constraints",
        "Model the ADAF accretion SED upper limit for a given efficiency and gas density"
      ]
    },
    {
      "id": "fermi",
      "name": "Fermi Paradox & Cosmology",
      "description": "Drake-equation Monte Carlo (deterministically seeded for reproducible hashes), Great Filter analysis, and cosmological context. Speculative-register tools are flagged as such in compliance_flags.",
      "tags": [
        "Drake equation",
        "Great Filter",
        "Fermi paradox",
        "cosmology"
      ],
      "examples": [
        "Run a seeded Drake-equation Monte Carlo and report P(N<1)",
        "Analyse Great Filter placement scenarios"
      ]
    },
    {
      "id": "seti",
      "name": "SETI Signal Characterisation",
      "description": "Radio-SETI detection sensitivity and infrared-excess (Dyson-sphere) checks over Omega Centauri targets.",
      "tags": [
        "SETI",
        "radio",
        "IR excess",
        "technosignature"
      ],
      "examples": [
        "Compute radio-SETI detection SNR for an EIRP and distance"
      ]
    },
    {
      "id": "mth",
      "name": "Macro Transcension Hypothesis",
      "description": "Bekenstein-Landauer-Lloyd computation limits and infall-survival modelling — speculative-register engineering extrapolations, flagged accordingly.",
      "tags": [
        "MTH",
        "Bekenstein bound",
        "Landauer",
        "compute limits"
      ],
      "examples": [
        "Estimate the Bekenstein-Landauer compute ceiling for a given mass-energy budget"
      ]
    },
    {
      "id": "kardashev",
      "name": "Kardashev-Scale Energy",
      "description": "Kardashev-scale energy-extraction metrics and Blandford-Znajek power for the candidate black hole — speculative register.",
      "tags": [
        "Kardashev",
        "Blandford-Znajek",
        "energy extraction"
      ],
      "examples": [
        "Compute Blandford-Znajek power for a spin and field strength"
      ]
    }
  ],
  "license": {
    "code": "MIT",
    "prose": "CC BY 4.0",
    "data": "CC0"
  },
  "updated": "2026-06-14"
}