{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:TF6W3TMJK22TSA7JRYPMCTL4EL","short_pith_number":"pith:TF6W3TMJ","schema_version":"1.0","canonical_sha256":"997d6dcd8956b53903e98e1ec14d7c22ea6a64ca07441e0f5b385593dde205d7","source":{"kind":"arxiv","id":"2103.06895","version":1},"attestation_state":"computed","paper":{"title":"On the construction of asymptotically flat initial data in scalar-tensor effective field theory","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Aron D Kovacs","submitted_at":"2021-03-11T19:00:02Z","abstract_excerpt":"We study the constraint equations for a class of scalar-tensor effective field theories of gravity, including the operators up to $4$ derivatives in the action ($4\\partial$ST). We extend the conformal transverse traceless and conformal thin sandwich methods of General Relativity to rewrite the constraint equations of the scalar-tensor theory as a set of elliptic partial differential equations. It is shown that, at weak coupling, a unique solution exists to the corresponding elliptic boundary value problems on asymptotically Euclidean initial slices under similar conditions as in the case of Ge"},"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":"2103.06895","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2021-03-11T19:00:02Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"4042a49985a04549e4a6bed7d72323502258221d26da6b5f520b996fc19ad310","abstract_canon_sha256":"fd95b1005a5637a5eed2fb4c735335d009c62414bba42b07bdbc5da710140edc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:22:26.500673Z","signature_b64":"al3TyyjLvYeQEOPqcfnYxAdd3WYxvesQ0KqJGvd0keGuvr0dl1MriXgMGfhzjrizc/M6k2MNQ5fNipvIMGhyBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"997d6dcd8956b53903e98e1ec14d7c22ea6a64ca07441e0f5b385593dde205d7","last_reissued_at":"2026-07-05T02:22:26.500190Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:22:26.500190Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the construction of asymptotically flat initial data in scalar-tensor effective field theory","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Aron D Kovacs","submitted_at":"2021-03-11T19:00:02Z","abstract_excerpt":"We study the constraint equations for a class of scalar-tensor effective field theories of gravity, including the operators up to $4$ derivatives in the action ($4\\partial$ST). We extend the conformal transverse traceless and conformal thin sandwich methods of General Relativity to rewrite the constraint equations of the scalar-tensor theory as a set of elliptic partial differential equations. It is shown that, at weak coupling, a unique solution exists to the corresponding elliptic boundary value problems on asymptotically Euclidean initial slices under similar conditions as in the case of Ge"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2103.06895","kind":"arxiv","version":1},"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/2103.06895/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":"2103.06895","created_at":"2026-07-05T02:22:26.500247+00:00"},{"alias_kind":"arxiv_version","alias_value":"2103.06895v1","created_at":"2026-07-05T02:22:26.500247+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2103.06895","created_at":"2026-07-05T02:22:26.500247+00:00"},{"alias_kind":"pith_short_12","alias_value":"TF6W3TMJK22T","created_at":"2026-07-05T02:22:26.500247+00:00"},{"alias_kind":"pith_short_16","alias_value":"TF6W3TMJK22TSA7J","created_at":"2026-07-05T02:22:26.500247+00:00"},{"alias_kind":"pith_short_8","alias_value":"TF6W3TMJ","created_at":"2026-07-05T02:22:26.500247+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2607.01177","citing_title":"Preheating and oscillon formation in Einstein-scalar-Gauss-Bonnet gravity","ref_index":127,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TF6W3TMJK22TSA7JRYPMCTL4EL","json":"https://pith.science/pith/TF6W3TMJK22TSA7JRYPMCTL4EL.json","graph_json":"https://pith.science/api/pith-number/TF6W3TMJK22TSA7JRYPMCTL4EL/graph.json","events_json":"https://pith.science/api/pith-number/TF6W3TMJK22TSA7JRYPMCTL4EL/events.json","paper":"https://pith.science/paper/TF6W3TMJ"},"agent_actions":{"view_html":"https://pith.science/pith/TF6W3TMJK22TSA7JRYPMCTL4EL","download_json":"https://pith.science/pith/TF6W3TMJK22TSA7JRYPMCTL4EL.json","view_paper":"https://pith.science/paper/TF6W3TMJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2103.06895&json=true","fetch_graph":"https://pith.science/api/pith-number/TF6W3TMJK22TSA7JRYPMCTL4EL/graph.json","fetch_events":"https://pith.science/api/pith-number/TF6W3TMJK22TSA7JRYPMCTL4EL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TF6W3TMJK22TSA7JRYPMCTL4EL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TF6W3TMJK22TSA7JRYPMCTL4EL/action/storage_attestation","attest_author":"https://pith.science/pith/TF6W3TMJK22TSA7JRYPMCTL4EL/action/author_attestation","sign_citation":"https://pith.science/pith/TF6W3TMJK22TSA7JRYPMCTL4EL/action/citation_signature","submit_replication":"https://pith.science/pith/TF6W3TMJK22TSA7JRYPMCTL4EL/action/replication_record"}},"created_at":"2026-07-05T02:22:26.500247+00:00","updated_at":"2026-07-05T02:22:26.500247+00:00"}