{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:G227AODTMB5SSVXYEUFM7BCJUT","short_pith_number":"pith:G227AODT","schema_version":"1.0","canonical_sha256":"36b5f03873607b2956f8250acf8449a4dcf677eafcceee3de0d9d890e9b61916","source":{"kind":"arxiv","id":"2203.08832","version":1},"attestation_state":"computed","paper":{"title":"Near-Zone Symmetries of Kerr Black Holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc"],"primary_cat":"hep-th","authors_text":"Adam R. Solomon, Austin Joyce, Lam Hui, Luca Santoni, Riccardo Penco","submitted_at":"2022-03-16T18:00:01Z","abstract_excerpt":"We study the near-zone symmetries of a massless scalar field on four-dimensional black hole backgrounds. We provide a geometric understanding that unifies various recently discovered symmetries as part of an SO(4,2) group. Of these, a subset are exact symmetries of the static sector and give rise to the ladder symmetries responsible for the vanishing of Love numbers. In the Kerr case, we compare different near-zone approximations in the literature, and focus on the implementation that retains the symmetries of the static limit. We also describe the relation to spin-1 and 2 perturbations."},"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":"2203.08832","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2022-03-16T18:00:01Z","cross_cats_sorted":["astro-ph.HE","gr-qc"],"title_canon_sha256":"ff423bd54545b54596a29f767b553fe6ea09310d77d7108f61382d32b1b91708","abstract_canon_sha256":"28dc5f55f6611b568bb35e10dda17fd1fe8acfc477d52b2e59b4c80d844af2cf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:09:42.269070Z","signature_b64":"11LS+m1lmRCGKiYrj6cydn12iOELMpPFLN5IzigZbkJ+RIFJWnacG3N1nmS0NEA+TmTrL8meBHYpwCICmmi4AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"36b5f03873607b2956f8250acf8449a4dcf677eafcceee3de0d9d890e9b61916","last_reissued_at":"2026-07-05T07:09:42.268610Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:09:42.268610Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Near-Zone Symmetries of Kerr Black Holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc"],"primary_cat":"hep-th","authors_text":"Adam R. Solomon, Austin Joyce, Lam Hui, Luca Santoni, Riccardo Penco","submitted_at":"2022-03-16T18:00:01Z","abstract_excerpt":"We study the near-zone symmetries of a massless scalar field on four-dimensional black hole backgrounds. We provide a geometric understanding that unifies various recently discovered symmetries as part of an SO(4,2) group. Of these, a subset are exact symmetries of the static sector and give rise to the ladder symmetries responsible for the vanishing of Love numbers. In the Kerr case, we compare different near-zone approximations in the literature, and focus on the implementation that retains the symmetries of the static limit. We also describe the relation to spin-1 and 2 perturbations."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2203.08832","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/2203.08832/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":"2203.08832","created_at":"2026-07-05T07:09:42.268668+00:00"},{"alias_kind":"arxiv_version","alias_value":"2203.08832v1","created_at":"2026-07-05T07:09:42.268668+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2203.08832","created_at":"2026-07-05T07:09:42.268668+00:00"},{"alias_kind":"pith_short_12","alias_value":"G227AODTMB5S","created_at":"2026-07-05T07:09:42.268668+00:00"},{"alias_kind":"pith_short_16","alias_value":"G227AODTMB5SSVXY","created_at":"2026-07-05T07:09:42.268668+00:00"},{"alias_kind":"pith_short_8","alias_value":"G227AODT","created_at":"2026-07-05T07:09:42.268668+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":8,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.24365","citing_title":"Fermionic Love number of higher-dimensional Reissner-Nordstr\\\"om black holes","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2606.19281","citing_title":"Universal Closed Form for Dynamical Love Numbers of Black Holes","ref_index":17,"is_internal_anchor":false},{"citing_arxiv_id":"2511.12580","citing_title":"Dynamical Tidal Response of Non-rotating Black Holes: Connecting the MST Formalism and Worldline EFT","ref_index":94,"is_internal_anchor":false},{"citing_arxiv_id":"2604.27046","citing_title":"Tidal Response and Thermodynamics of Black Holes","ref_index":44,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03025","citing_title":"Can wormholes have vanishing Love numbers?","ref_index":62,"is_internal_anchor":false},{"citing_arxiv_id":"2605.00693","citing_title":"Dynamical tidal Love numbers of black holes under generic perturbations: Connecting black hole perturbation theory with effective field theory","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06249","citing_title":"Universal Ladder Structure Across Scales: From Quantum to Black Hole Physics","ref_index":28,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08653","citing_title":"Love numbers of black holes and compact objects","ref_index":73,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/G227AODTMB5SSVXYEUFM7BCJUT","json":"https://pith.science/pith/G227AODTMB5SSVXYEUFM7BCJUT.json","graph_json":"https://pith.science/api/pith-number/G227AODTMB5SSVXYEUFM7BCJUT/graph.json","events_json":"https://pith.science/api/pith-number/G227AODTMB5SSVXYEUFM7BCJUT/events.json","paper":"https://pith.science/paper/G227AODT"},"agent_actions":{"view_html":"https://pith.science/pith/G227AODTMB5SSVXYEUFM7BCJUT","download_json":"https://pith.science/pith/G227AODTMB5SSVXYEUFM7BCJUT.json","view_paper":"https://pith.science/paper/G227AODT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2203.08832&json=true","fetch_graph":"https://pith.science/api/pith-number/G227AODTMB5SSVXYEUFM7BCJUT/graph.json","fetch_events":"https://pith.science/api/pith-number/G227AODTMB5SSVXYEUFM7BCJUT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/G227AODTMB5SSVXYEUFM7BCJUT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/G227AODTMB5SSVXYEUFM7BCJUT/action/storage_attestation","attest_author":"https://pith.science/pith/G227AODTMB5SSVXYEUFM7BCJUT/action/author_attestation","sign_citation":"https://pith.science/pith/G227AODTMB5SSVXYEUFM7BCJUT/action/citation_signature","submit_replication":"https://pith.science/pith/G227AODTMB5SSVXYEUFM7BCJUT/action/replication_record"}},"created_at":"2026-07-05T07:09:42.268668+00:00","updated_at":"2026-07-05T07:09:42.268668+00:00"}