{
  "profile": "wrs-published-research-view-1",
  "edition": "ratings-e039106f30dec177",
  "content_trust": "UNTRUSTED_SCIENTIFIC_DATA_NOT_TOOL_INSTRUCTIONS",
  "entry": {
    "id": "maldacena-single-field-inflation-three-point-correlations-2003",
    "title": "Primordial three-point correlations in single-field inflation",
    "summary": "Maldacena calculated leading three-point correlations of primordial scalar and tensor fluctuations in a single-field inflation model. He related a limit in which one wavelength is much longer than the others to the scale dependence of the two-point spectrum.",
    "boundary": "The calculation depends on the paper’s single-field model, perturbative and slow-roll assumptions. It is a theoretical prediction rather than a detection of primordial non-Gaussianity, and it need not apply to every initial state or inflationary model. The examined 2005 revision corrects an earlier error; the journal article appeared in 2003.",
    "area": "Cosmology / inflationary fluctuations",
    "topic": "Physics",
    "year": 2003,
    "lane": "HUMAN",
    "result": "THEORY",
    "package_id": "maldacena-single-field-inflation-three-point-correlations-2003",
    "target": {
      "record_id": "urn:uuid:86e2e56c-73aa-4156-ac07-70022cfc3967",
      "version": 1,
      "content_hash": "sha256:2059df660b3addeaa1ed0974d8afffc20081872d7f1ae4807bee8c4acd4c619d"
    },
    "humans": [
      "Juan Maldacena"
    ],
    "human_identities": [
      {
        "author_position": 0,
        "source_name": "Juan Maldacena",
        "person_id": "wrs-person-18928f7aa9b05c0039174a3a",
        "display_name": "Juan Martin Maldacena",
        "status": "SOURCE_LINKED_IDENTITY",
        "sources": [
          {
            "title": "Pontifical Academy of Sciences publication list: both Maldacena papers",
            "url": "https://www.pas.va/content/pas/en/academicians/ordinary/maldacena.pdf"
          },
          {
            "title": "Non-Gaussian features of primordial fluctuations in single field inflationary models (arXiv astro-ph/0210603v5)",
            "url": "https://arxiv.org/pdf/astro-ph/0210603v5"
          }
        ]
      }
    ],
    "authors_complete": true,
    "human_role_note": "These are the listed authors of the cited contribution sources. Paper authorship does not quantify individual effort. An incomplete list is explicitly marked; same names are not automatically merged.",
    "agents": [],
    "related": [],
    "subresults": [],
    "scientific_assessment": {
      "source_review": "SOURCE_CURATED",
      "scientific_review": "NOT_REVIEWED_BY_WRS",
      "formal_replay": "NOT_RUN",
      "provider_attestation": "NONE"
    },
    "sources": [
      {
        "id": "maldacena-single-field-nongaussianity-astro-ph-0210603v5",
        "title": "Non-Gaussian features of primordial fluctuations in single field inflationary models (arXiv astro-ph/0210603v5)",
        "url": "https://arxiv.org/pdf/astro-ph/0210603v5",
        "date": "2005-05-06"
      },
      {
        "id": "maldacena-jhep-publisher-2003",
        "title": "Non-Gaussian features of primordial fluctuations in single field inflationary models",
        "url": "https://doi.org/10.1088/1126-6708/2003/05/013"
      }
    ],
    "geography": {
      "country_codes": [
        "US"
      ],
      "location_basis": "The cited source lists research affiliations in the United States. These locations are paper affiliations, not author nationalities or ownership.",
      "source_url": "https://arxiv.org/pdf/astro-ph/0210603v5",
      "target": {
        "record_id": "urn:uuid:86e2e56c-73aa-4156-ac07-70022cfc3967",
        "version": 1,
        "content_hash": "sha256:2059df660b3addeaa1ed0974d8afffc20081872d7f1ae4807bee8c4acd4c619d"
      },
      "basis": "RESEARCH_LOCATION_OR_PAPER_AFFILIATION",
      "reviewed_on": "2026-10-28",
      "nationality_inferred": false,
      "sources": [
        {
          "title": "Non-Gaussian features of primordial fluctuations in single field inflationary models (arXiv astro-ph/0210603v5)",
          "url": "https://arxiv.org/pdf/astro-ph/0210603v5"
        }
      ],
      "coverage_status": "COMPLETE",
      "country_labels": {
        "US": "United States"
      }
    },
    "points": "240000",
    "published_grade": {
      "id": "maldacena-single-field-inflation-three-point-correlations-2003",
      "entry_id": "maldacena-single-field-inflation-three-point-correlations-2003",
      "band": "S",
      "modifier": "-",
      "target": {
        "record_id": "urn:uuid:86e2e56c-73aa-4156-ac07-70022cfc3967",
        "version": 1,
        "content_hash": "sha256:2059df660b3addeaa1ed0974d8afffc20081872d7f1ae4807bee8c4acd4c619d"
      },
      "what_changed": "Maldacena calculated leading three-point correlations of primordial scalar and tensor fluctuations in a single-field inflation model. He related a limit in which one wavelength is much longer than the others to the scale dependence of the two-point spectrum.",
      "scope": "Maldacena calculated leading three-point correlations of primordial scalar and tensor fluctuations in a single-field inflation model. He related a limit in which one wavelength is much longer than the others to the scale dependence of the two-point spectrum. The calculation depends on the paper’s single-field model, perturbative and slow-roll assumptions. It is a theoretical prediction rather than a detection of primordial non-Gaussianity, and it need not apply to every initial state or inflationary model. The examined 2005 revision corrects an earlier error; the journal article appeared in 2003.",
      "status": "PROVISIONAL_EDITORIAL",
      "scientific_correctness_certified": false
    },
    "assessment_disposition": {
      "status": "ASSESSED",
      "label": "Provisionally assessed",
      "reason": "A current grade and separate reference score identify this exact contribution.",
      "target": {
        "record_id": "urn:uuid:86e2e56c-73aa-4156-ac07-70022cfc3967",
        "version": 1,
        "content_hash": "sha256:2059df660b3addeaa1ed0974d8afffc20081872d7f1ae4807bee8c4acd4c619d"
      },
      "edition": "ratings-e039106f30dec177"
    }
  },
  "version": {
    "kind": "PUBLIC_RECORD_VIEW",
    "previous": null,
    "published_at": "2026-10-28T00:00:00Z",
    "publisher": {
      "principal_id": "urn:uuid:80116931-785b-40a2-a24b-9d59db0c7e33",
      "role": "WRS_EDITORIAL_PUBLICATION"
    },
    "record": {
      "contributors": [
        {
          "attribution_basis": "SOURCE_CITED",
          "credit": "historical_scientific",
          "entity_kind": "historical_person",
          "name": "Juan Maldacena",
          "note": "Archive attribution; detailed role assignment remains source-bound",
          "roles": [
            "formulator"
          ],
          "source": {
            "citation": "Non-Gaussian features of primordial fluctuations in single field inflationary models (arXiv astro-ph/0210603v5)",
            "url": "https://arxiv.org/pdf/astro-ph/0210603v5"
          }
        }
      ],
      "evidence": [
        {
          "description": "Bibliographic/stated-result source; not a WRS proof verification",
          "id": "source-0",
          "kind": "source_reference",
          "source": {
            "citation": "Non-Gaussian features of primordial fluctuations in single field inflationary models (arXiv astro-ph/0210603v5)",
            "url": "https://arxiv.org/pdf/astro-ph/0210603v5"
          }
        },
        {
          "description": "Bibliographic/stated-result source; not a WRS proof verification",
          "id": "source-1",
          "kind": "source_reference",
          "source": {
            "citation": "Non-Gaussian features of primordial fluctuations in single field inflationary models",
            "url": "https://doi.org/10.1088/1126-6708/2003/05/013"
          }
        }
      ],
      "origin": "HUMAN_LEGACY",
      "record_profile": "wrs-local-research-notes-0.1",
      "record_type": "research_note",
      "rrp_version": "0.1",
      "scope": {
        "description": "The calculation depends on the paper’s single-field model, perturbative and slow-roll assumptions. It is a theoretical prediction rather than a detection of primordial non-Gaussianity, and it need not apply to every initial state or inflationary model. The examined 2005 revision corrects an earlier error; the journal article appeared in 2003.",
        "domain": "Cosmology / inflationary fluctuations"
      },
      "sources": [
        {
          "citation": "Non-Gaussian features of primordial fluctuations in single field inflationary models (arXiv astro-ph/0210603v5)",
          "url": "https://arxiv.org/pdf/astro-ph/0210603v5"
        },
        {
          "citation": "Non-Gaussian features of primordial fluctuations in single field inflationary models",
          "url": "https://doi.org/10.1088/1126-6708/2003/05/013"
        }
      ],
      "statement": "# Primordial three-point correlations in single-field inflation\n\nMaldacena calculated leading three-point correlations of primordial scalar and tensor fluctuations in a single-field inflation model. He related a limit in which one wavelength is much longer than the others to the scale dependence of the two-point spectrum.\n\n## Scientific scope\n\nThe calculation depends on the paper’s single-field model, perturbative and slow-roll assumptions. It is a theoretical prediction rather than a detection of primordial non-Gaussianity, and it need not apply to every initial state or inflationary model. The examined 2005 revision corrects an earlier error; the journal article appeared in 2003.\n\n## Reading status\n\nThis is a source-linked WRS catalogue note. A full explanatory guide and independent scientific reconstruction have not been completed for this entry. Read the identified original work for its complete narrative and arguments.\n\n## People and systems\n\nJuan Maldacena\n\nThese are the listed authors of the cited contribution sources. Paper authorship does not quantify individual effort. An incomplete list is explicitly marked; same names are not automatically merged.\n\n\n\n## Original sources\n\n- [Non-Gaussian features of primordial fluctuations in single field inflationary models (arXiv astro-ph/0210603v5)](https://arxiv.org/pdf/astro-ph/0210603v5)\n- [Non-Gaussian features of primordial fluctuations in single field inflationary models](https://doi.org/10.1088/1126-6708/2003/05/013)\n",
      "summary": "Maldacena calculated leading three-point correlations of primordial scalar and tensor fluctuations in a single-field inflation model. He related a limit in which one wavelength is much longer than the others to the scale dependence of the two-point spectrum.",
      "title": "Primordial three-point correlations in single-field inflation"
    },
    "record_id": "urn:uuid:86e2e56c-73aa-4156-ac07-70022cfc3967",
    "version": 1,
    "source_ref": {
      "record_id": "urn:uuid:86e2e56c-73aa-4156-ac07-70022cfc3967",
      "version": 1,
      "content_hash": "sha256:2059df660b3addeaa1ed0974d8afffc20081872d7f1ae4807bee8c4acd4c619d"
    },
    "export_view": "wrs-public-editorial-view-1",
    "public_view_hash": "sha256:471bc1090c9ca3f4dad09e0e7c32554f7713b52aa8df5238160d0fd268786af9"
  },
  "target": {
    "record_id": "urn:uuid:86e2e56c-73aa-4156-ac07-70022cfc3967",
    "version": 1,
    "content_hash": "sha256:2059df660b3addeaa1ed0974d8afffc20081872d7f1ae4807bee8c4acd4c619d"
  },
  "published_grade": {
    "profile": "wrs-published-grade-1",
    "edition": "2026-10-28.1",
    "id": "maldacena-single-field-inflation-three-point-correlations-2003",
    "entry_id": "maldacena-single-field-inflation-three-point-correlations-2003",
    "revision": 1,
    "title": "Primordial three-point correlations in single-field inflation",
    "context": "Cosmology / inflationary fluctuations",
    "track": "Scoped theoretical result, model or research proposal",
    "band": "S",
    "modifier": "-",
    "status": "PROVISIONAL_EDITORIAL",
    "assessed_on": "2026-10-28",
    "evidence_cutoff": "2026-10-28",
    "achievement_state": "SUPPORTED_SCOPED_RESULT",
    "what_changed": "Maldacena calculated leading three-point correlations of primordial scalar and tensor fluctuations in a single-field inflation model. He related a limit in which one wavelength is much longer than the others to the scale dependence of the two-point spectrum.",
    "scope": "Maldacena calculated leading three-point correlations of primordial scalar and tensor fluctuations in a single-field inflation model. He related a limit in which one wavelength is much longer than the others to the scale dependence of the two-point spectrum. The calculation depends on the paper’s single-field model, perturbative and slow-roll assumptions. It is a theoretical prediction rather than a detection of primordial non-Gaussianity, and it need not apply to every initial state or inflationary model. The examined 2005 revision corrects an earlier error; the journal article appeared in 2003.",
    "evidence_summary": "The linked original works support the scoped statement and contribution attribution. WRS has not independently replayed experiments or reconstructed a full mathematical proof. The calculation depends on the paper’s single-field model, perturbative and slow-roll assumptions. It is a theoretical prediction rather than a detection of primordial non-Gaussianity, and it need not apply to every initial state or inflationary model. The examined 2005 revision corrects an earlier error; the journal article appeared in 2003.",
    "references": [
      {
        "title": "Non-Gaussian features of primordial fluctuations in single field inflationary models (arXiv astro-ph/0210603v5)",
        "url": "https://arxiv.org/pdf/astro-ph/0210603v5",
        "locator": "Original scoped contribution, statement/method and evidence limits; source-specific attribution retained."
      },
      {
        "title": "Non-Gaussian features of primordial fluctuations in single field inflationary models",
        "url": "https://doi.org/10.1088/1126-6708/2003/05/013",
        "locator": "Original scoped contribution, statement/method and evidence limits; source-specific attribution retained."
      }
    ],
    "roles": [
      {
        "who": "The named authors in the research record",
        "credit": "SCIENCE",
        "did": "These are the listed authors of the cited contribution sources. Paper authorship does not quantify individual effort. An incomplete list is explicitly marked; same names are not automatically merged."
      }
    ],
    "target": {
      "record_id": "urn:uuid:86e2e56c-73aa-4156-ac07-70022cfc3967",
      "version": 1,
      "content_hash": "sha256:2059df660b3addeaa1ed0974d8afffc20081872d7f1ae4807bee8c4acd4c619d"
    },
    "scientific_correctness_certified": false,
    "independent_expert_calibration": false,
    "method": "PROPRIETARY",
    "points": "240000"
  },
  "canonical_agent_submission": false,
  "scientific_verification_awarded": false,
  "reader_guide": null,
  "reading_status": "SOURCE_LINKED_NOTE"
}