{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:SJY4XRIXOMX2QBLEWD2PYPMV4B","short_pith_number":"pith:SJY4XRIX","schema_version":"1.0","canonical_sha256":"9271cbc517732fa80564b0f4fc3d95e04ae9c865d22703c979eac046ec7df9a6","source":{"kind":"arxiv","id":"1905.08816","version":2},"attestation_state":"computed","paper":{"title":"To Positivity and Beyond, where Higgs-Dilaton Inflation has never gone before","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-th"],"primary_cat":"hep-ph","authors_text":"Anna Tokareva, Inar Timiryasov, Mario Herrero-Valea","submitted_at":"2019-05-21T18:00:06Z","abstract_excerpt":"We study the consequences of (beyond) positivity of scattering amplitudes in the effective field theory description of the Higgs-Dilaton inflationary model. By requiring the EFT to be compatible with a unitary, causal, local and Lorentz invariant UV completion, we derive constraints on the Wilson coefficients of the first higher order derivative operators. We show that the values allowed by the constraints are consistent with the phenomenological applications of the Higgs-Dilaton model."},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1905.08816","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2019-05-21T18:00:06Z","cross_cats_sorted":["gr-qc","hep-th"],"title_canon_sha256":"4b908571770df3807c1ff6a4c16005644833068a42529c80e0cd4b90eca4a73e","abstract_canon_sha256":"60d47573fa18cad17b77d47848b42b723be9ab99b0aa40626832f8614ed2ca34"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:33:12.605035Z","signature_b64":"JxSCeOIaelVVguqbomJJu+uuWozy8syK39IG4QMa24iVmz3ObnTZe9ZkXSpOGeLmRVzYDg92SHevUtl3K1jHBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9271cbc517732fa80564b0f4fc3d95e04ae9c865d22703c979eac046ec7df9a6","last_reissued_at":"2026-07-05T00:33:12.604570Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:33:12.604570Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"To Positivity and Beyond, where Higgs-Dilaton Inflation has never gone before","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-th"],"primary_cat":"hep-ph","authors_text":"Anna Tokareva, Inar Timiryasov, Mario Herrero-Valea","submitted_at":"2019-05-21T18:00:06Z","abstract_excerpt":"We study the consequences of (beyond) positivity of scattering amplitudes in the effective field theory description of the Higgs-Dilaton inflationary model. By requiring the EFT to be compatible with a unitary, causal, local and Lorentz invariant UV completion, we derive constraints on the Wilson coefficients of the first higher order derivative operators. We show that the values allowed by the constraints are consistent with the phenomenological applications of the Higgs-Dilaton model."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1905.08816","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1905.08816/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1905.08816","created_at":"2026-07-05T00:33:12.604637+00:00"},{"alias_kind":"arxiv_version","alias_value":"1905.08816v2","created_at":"2026-07-05T00:33:12.604637+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1905.08816","created_at":"2026-07-05T00:33:12.604637+00:00"},{"alias_kind":"pith_short_12","alias_value":"SJY4XRIXOMX2","created_at":"2026-07-05T00:33:12.604637+00:00"},{"alias_kind":"pith_short_16","alias_value":"SJY4XRIXOMX2QBLE","created_at":"2026-07-05T00:33:12.604637+00:00"},{"alias_kind":"pith_short_8","alias_value":"SJY4XRIX","created_at":"2026-07-05T00:33:12.604637+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.19283","citing_title":"A Dispersive Bootstrap for the Virasoro-Shapiro Amplitude","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"2509.06630","citing_title":"Positivity bounds from thermal field theory entropy","ref_index":13,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15235","citing_title":"Sampling the Graviton Pole and Deprojecting the Swampland","ref_index":10,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SJY4XRIXOMX2QBLEWD2PYPMV4B","json":"https://pith.science/pith/SJY4XRIXOMX2QBLEWD2PYPMV4B.json","graph_json":"https://pith.science/api/pith-number/SJY4XRIXOMX2QBLEWD2PYPMV4B/graph.json","events_json":"https://pith.science/api/pith-number/SJY4XRIXOMX2QBLEWD2PYPMV4B/events.json","paper":"https://pith.science/paper/SJY4XRIX"},"agent_actions":{"view_html":"https://pith.science/pith/SJY4XRIXOMX2QBLEWD2PYPMV4B","download_json":"https://pith.science/pith/SJY4XRIXOMX2QBLEWD2PYPMV4B.json","view_paper":"https://pith.science/paper/SJY4XRIX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1905.08816&json=true","fetch_graph":"https://pith.science/api/pith-number/SJY4XRIXOMX2QBLEWD2PYPMV4B/graph.json","fetch_events":"https://pith.science/api/pith-number/SJY4XRIXOMX2QBLEWD2PYPMV4B/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SJY4XRIXOMX2QBLEWD2PYPMV4B/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SJY4XRIXOMX2QBLEWD2PYPMV4B/action/storage_attestation","attest_author":"https://pith.science/pith/SJY4XRIXOMX2QBLEWD2PYPMV4B/action/author_attestation","sign_citation":"https://pith.science/pith/SJY4XRIXOMX2QBLEWD2PYPMV4B/action/citation_signature","submit_replication":"https://pith.science/pith/SJY4XRIXOMX2QBLEWD2PYPMV4B/action/replication_record"}},"created_at":"2026-07-05T00:33:12.604637+00:00","updated_at":"2026-07-05T00:33:12.604637+00:00"}