{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:INUS5CC25X57ES4W52C4QOMNL3","short_pith_number":"pith:INUS5CC2","schema_version":"1.0","canonical_sha256":"43692e885aedfbf24b96ee85c8398d5edb7bef7bf1d3c5f0f9c1ec39afc5f949","source":{"kind":"arxiv","id":"2206.12597","version":2},"attestation_state":"computed","paper":{"title":"Metric reconstruction from celestial multipoles","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Ali Seraj, Geoffrey Comp\\`ere, Roberto Oliveri","submitted_at":"2022-06-25T08:38:23Z","abstract_excerpt":"The most general vacuum solution to Einstein's field equations with no incoming radiation can be constructed perturbatively from two infinite sets of canonical multipole moments, which are found to be mapped into each other under gravitational electric-magnetic duality at the non-linear level. We demonstrate that in non-radiative regions such spacetimes are completely characterized by a set of conserved celestial charges that consist of the Geroch-Hansen multipole moments, the generalized BMS charges and additional celestial multipoles accounting for subleading memory effects. Transitions amon"},"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":"2206.12597","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2022-06-25T08:38:23Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"1351e3569ca9d48b9d7898003833d770d9d05291711b46b10060b4276f37f493","abstract_canon_sha256":"0d08aa83fccf11c5d4eb75f0148cc6b7ffba77421eade7284cc2a74fe778d711"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:13:07.459026Z","signature_b64":"PJTRymuA2gl1AiCHEVcj/TwJWZzz9rQRwKdWpVQt/EhsYOC2HmqsMJb8Iod+uVJGn4aYOyaNg5kKIUvXdUdlAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"43692e885aedfbf24b96ee85c8398d5edb7bef7bf1d3c5f0f9c1ec39afc5f949","last_reissued_at":"2026-07-05T05:13:07.458545Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:13:07.458545Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Metric reconstruction from celestial multipoles","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Ali Seraj, Geoffrey Comp\\`ere, Roberto Oliveri","submitted_at":"2022-06-25T08:38:23Z","abstract_excerpt":"The most general vacuum solution to Einstein's field equations with no incoming radiation can be constructed perturbatively from two infinite sets of canonical multipole moments, which are found to be mapped into each other under gravitational electric-magnetic duality at the non-linear level. We demonstrate that in non-radiative regions such spacetimes are completely characterized by a set of conserved celestial charges that consist of the Geroch-Hansen multipole moments, the generalized BMS charges and additional celestial multipoles accounting for subleading memory effects. Transitions amon"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2206.12597","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/2206.12597/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":"2206.12597","created_at":"2026-07-05T05:13:07.458603+00:00"},{"alias_kind":"arxiv_version","alias_value":"2206.12597v2","created_at":"2026-07-05T05:13:07.458603+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2206.12597","created_at":"2026-07-05T05:13:07.458603+00:00"},{"alias_kind":"pith_short_12","alias_value":"INUS5CC25X57","created_at":"2026-07-05T05:13:07.458603+00:00"},{"alias_kind":"pith_short_16","alias_value":"INUS5CC25X57ES4W","created_at":"2026-07-05T05:13:07.458603+00:00"},{"alias_kind":"pith_short_8","alias_value":"INUS5CC2","created_at":"2026-07-05T05:13:07.458603+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.02722","citing_title":"Asymptotically-FLRW$_3$ spacetimes","ref_index":132,"is_internal_anchor":false},{"citing_arxiv_id":"2604.12854","citing_title":"Mixed-helicity bracket of celestial symmetries","ref_index":114,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13362","citing_title":"Quasi-Local Celestial Charges and Multipoles","ref_index":40,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/INUS5CC25X57ES4W52C4QOMNL3","json":"https://pith.science/pith/INUS5CC25X57ES4W52C4QOMNL3.json","graph_json":"https://pith.science/api/pith-number/INUS5CC25X57ES4W52C4QOMNL3/graph.json","events_json":"https://pith.science/api/pith-number/INUS5CC25X57ES4W52C4QOMNL3/events.json","paper":"https://pith.science/paper/INUS5CC2"},"agent_actions":{"view_html":"https://pith.science/pith/INUS5CC25X57ES4W52C4QOMNL3","download_json":"https://pith.science/pith/INUS5CC25X57ES4W52C4QOMNL3.json","view_paper":"https://pith.science/paper/INUS5CC2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2206.12597&json=true","fetch_graph":"https://pith.science/api/pith-number/INUS5CC25X57ES4W52C4QOMNL3/graph.json","fetch_events":"https://pith.science/api/pith-number/INUS5CC25X57ES4W52C4QOMNL3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/INUS5CC25X57ES4W52C4QOMNL3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/INUS5CC25X57ES4W52C4QOMNL3/action/storage_attestation","attest_author":"https://pith.science/pith/INUS5CC25X57ES4W52C4QOMNL3/action/author_attestation","sign_citation":"https://pith.science/pith/INUS5CC25X57ES4W52C4QOMNL3/action/citation_signature","submit_replication":"https://pith.science/pith/INUS5CC25X57ES4W52C4QOMNL3/action/replication_record"}},"created_at":"2026-07-05T05:13:07.458603+00:00","updated_at":"2026-07-05T05:13:07.458603+00:00"}