{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:RIFTVNTRZMAJFIPIFXZHFTZAZZ","short_pith_number":"pith:RIFTVNTR","schema_version":"1.0","canonical_sha256":"8a0b3ab671cb0092a1e82df272cf20ce44087d46e349ccfc7ae54e1241710748","source":{"kind":"arxiv","id":"2309.13656","version":3},"attestation_state":"computed","paper":{"title":"Pleban\\'ski-Demia\\'nski \\`a la Ehlers-Harrison: Exact Rotating and Accelerating Type I Black Holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Adolfo Cisterna, Jos\\'e Barrientos, Konstantinos Pallikaris","submitted_at":"2023-09-24T14:50:07Z","abstract_excerpt":"Recently, it was shown that type D black holes, encompassed in the large Pleban\\'ski--Demia\\'nski (PD) family, exhibit a wide class of algebraically general generalizations via the application of Ehlers and Harrison transformations. In this work, we first discuss some mathematical details behind the composition of such transformations, and next, we introduce a qualitative picture of the most general type I generalization of the PD family, dubbed ``Enhanced Pleban\\'ski--Demia\\'nski'' spacetime. We provide the exact form of the solution in the original PD coordinates, obtained via the simultaneo"},"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":"2309.13656","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2023-09-24T14:50:07Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"c57a22d835fa2a72da5439a535be5a72532ae263672c9e44923a6c578716a2ff","abstract_canon_sha256":"b961ca5db001fbb2efab0da37b55346040be953e9a78f66f501859217a34ff86"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:11:22.128000Z","signature_b64":"gLTc+gRPqda7nnrTm+Y8nbgWRDoEV0WoYDMyMkshsqqtikQ0RR0EyMaK4He9wJ7TahhM/jNhoW6tNstw9GOtCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8a0b3ab671cb0092a1e82df272cf20ce44087d46e349ccfc7ae54e1241710748","last_reissued_at":"2026-07-05T09:11:22.127583Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:11:22.127583Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Pleban\\'ski-Demia\\'nski \\`a la Ehlers-Harrison: Exact Rotating and Accelerating Type I Black Holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Adolfo Cisterna, Jos\\'e Barrientos, Konstantinos Pallikaris","submitted_at":"2023-09-24T14:50:07Z","abstract_excerpt":"Recently, it was shown that type D black holes, encompassed in the large Pleban\\'ski--Demia\\'nski (PD) family, exhibit a wide class of algebraically general generalizations via the application of Ehlers and Harrison transformations. In this work, we first discuss some mathematical details behind the composition of such transformations, and next, we introduce a qualitative picture of the most general type I generalization of the PD family, dubbed ``Enhanced Pleban\\'ski--Demia\\'nski'' spacetime. We provide the exact form of the solution in the original PD coordinates, obtained via the simultaneo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2309.13656","kind":"arxiv","version":3},"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/2309.13656/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":"2309.13656","created_at":"2026-07-05T09:11:22.127637+00:00"},{"alias_kind":"arxiv_version","alias_value":"2309.13656v3","created_at":"2026-07-05T09:11:22.127637+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2309.13656","created_at":"2026-07-05T09:11:22.127637+00:00"},{"alias_kind":"pith_short_12","alias_value":"RIFTVNTRZMAJ","created_at":"2026-07-05T09:11:22.127637+00:00"},{"alias_kind":"pith_short_16","alias_value":"RIFTVNTRZMAJFIPI","created_at":"2026-07-05T09:11:22.127637+00:00"},{"alias_kind":"pith_short_8","alias_value":"RIFTVNTR","created_at":"2026-07-05T09:11:22.127637+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.13679","citing_title":"Thermodynamics of charged and accelerating black holes","ref_index":19,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RIFTVNTRZMAJFIPIFXZHFTZAZZ","json":"https://pith.science/pith/RIFTVNTRZMAJFIPIFXZHFTZAZZ.json","graph_json":"https://pith.science/api/pith-number/RIFTVNTRZMAJFIPIFXZHFTZAZZ/graph.json","events_json":"https://pith.science/api/pith-number/RIFTVNTRZMAJFIPIFXZHFTZAZZ/events.json","paper":"https://pith.science/paper/RIFTVNTR"},"agent_actions":{"view_html":"https://pith.science/pith/RIFTVNTRZMAJFIPIFXZHFTZAZZ","download_json":"https://pith.science/pith/RIFTVNTRZMAJFIPIFXZHFTZAZZ.json","view_paper":"https://pith.science/paper/RIFTVNTR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2309.13656&json=true","fetch_graph":"https://pith.science/api/pith-number/RIFTVNTRZMAJFIPIFXZHFTZAZZ/graph.json","fetch_events":"https://pith.science/api/pith-number/RIFTVNTRZMAJFIPIFXZHFTZAZZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RIFTVNTRZMAJFIPIFXZHFTZAZZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RIFTVNTRZMAJFIPIFXZHFTZAZZ/action/storage_attestation","attest_author":"https://pith.science/pith/RIFTVNTRZMAJFIPIFXZHFTZAZZ/action/author_attestation","sign_citation":"https://pith.science/pith/RIFTVNTRZMAJFIPIFXZHFTZAZZ/action/citation_signature","submit_replication":"https://pith.science/pith/RIFTVNTRZMAJFIPIFXZHFTZAZZ/action/replication_record"}},"created_at":"2026-07-05T09:11:22.127637+00:00","updated_at":"2026-07-05T09:11:22.127637+00:00"}