{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:WXQATX2HVL5IVH7QWU22SOXGNU","short_pith_number":"pith:WXQATX2H","schema_version":"1.0","canonical_sha256":"b5e009df47aafa8a9ff0b535a93ae66d0c7457a202774921fb5d3bcfed3f8b97","source":{"kind":"arxiv","id":"2512.19542","version":3},"attestation_state":"computed","paper":{"title":"Dynamical axisymmetric compact objects in General Relativity","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Adolfo Cisterna, Jibril Ben Achour, Mokhtar Hassaine","submitted_at":"2025-12-22T16:25:59Z","abstract_excerpt":"The search for exact solutions describing asymptotically FLRW compact objects in General Relativity remains a challenging problem. Progress has largely been limited to the spherically symmetric case, with notable exceptions such as the Kerr--de Sitter and Thakurta solutions. In this work, we present two new results that advance the description of axisymmetric compact objects embedded in a cosmological background. First, we introduce a new solution-generating technique that allows for the construction of nonstationary, axisymmetric solutions of the self-interacting Einstein-scalar system. Using"},"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":"2512.19542","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/publicdomain/zero/1.0/","primary_cat":"gr-qc","submitted_at":"2025-12-22T16:25:59Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"b136a4af92cc3c812d42bccf007d456de443da3c83053cf63217fa0fecebe830","abstract_canon_sha256":"c81173e80b08b228b44c6ad9c5a396dd2511e3cf4de5f35e2a51ac0de191e3e3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-03T01:17:16.027713Z","signature_b64":"dd07o/wih06vXvIv+pNfz0v9/hDn/Et5JKpv1xDeXqllNRjjIkrwp+vqLwiQ6fphI0qlWwgW5YJ7/wPWFA+pCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b5e009df47aafa8a9ff0b535a93ae66d0c7457a202774921fb5d3bcfed3f8b97","last_reissued_at":"2026-07-03T01:17:16.027212Z","signature_status":"signed_v1","first_computed_at":"2026-07-03T01:17:16.027212Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dynamical axisymmetric compact objects in General Relativity","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Adolfo Cisterna, Jibril Ben Achour, Mokhtar Hassaine","submitted_at":"2025-12-22T16:25:59Z","abstract_excerpt":"The search for exact solutions describing asymptotically FLRW compact objects in General Relativity remains a challenging problem. Progress has largely been limited to the spherically symmetric case, with notable exceptions such as the Kerr--de Sitter and Thakurta solutions. In this work, we present two new results that advance the description of axisymmetric compact objects embedded in a cosmological background. First, we introduce a new solution-generating technique that allows for the construction of nonstationary, axisymmetric solutions of the self-interacting Einstein-scalar system. Using"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2512.19542","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/2512.19542/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":"2512.19542","created_at":"2026-07-03T01:17:16.027270+00:00"},{"alias_kind":"arxiv_version","alias_value":"2512.19542v3","created_at":"2026-07-03T01:17:16.027270+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2512.19542","created_at":"2026-07-03T01:17:16.027270+00:00"},{"alias_kind":"pith_short_12","alias_value":"WXQATX2HVL5I","created_at":"2026-07-03T01:17:16.027270+00:00"},{"alias_kind":"pith_short_16","alias_value":"WXQATX2HVL5IVH7Q","created_at":"2026-07-03T01:17:16.027270+00:00"},{"alias_kind":"pith_short_8","alias_value":"WXQATX2H","created_at":"2026-07-03T01:17:16.027270+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2601.08628","citing_title":"Magnetized dynamical black holes","ref_index":38,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WXQATX2HVL5IVH7QWU22SOXGNU","json":"https://pith.science/pith/WXQATX2HVL5IVH7QWU22SOXGNU.json","graph_json":"https://pith.science/api/pith-number/WXQATX2HVL5IVH7QWU22SOXGNU/graph.json","events_json":"https://pith.science/api/pith-number/WXQATX2HVL5IVH7QWU22SOXGNU/events.json","paper":"https://pith.science/paper/WXQATX2H"},"agent_actions":{"view_html":"https://pith.science/pith/WXQATX2HVL5IVH7QWU22SOXGNU","download_json":"https://pith.science/pith/WXQATX2HVL5IVH7QWU22SOXGNU.json","view_paper":"https://pith.science/paper/WXQATX2H","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2512.19542&json=true","fetch_graph":"https://pith.science/api/pith-number/WXQATX2HVL5IVH7QWU22SOXGNU/graph.json","fetch_events":"https://pith.science/api/pith-number/WXQATX2HVL5IVH7QWU22SOXGNU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WXQATX2HVL5IVH7QWU22SOXGNU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WXQATX2HVL5IVH7QWU22SOXGNU/action/storage_attestation","attest_author":"https://pith.science/pith/WXQATX2HVL5IVH7QWU22SOXGNU/action/author_attestation","sign_citation":"https://pith.science/pith/WXQATX2HVL5IVH7QWU22SOXGNU/action/citation_signature","submit_replication":"https://pith.science/pith/WXQATX2HVL5IVH7QWU22SOXGNU/action/replication_record"}},"created_at":"2026-07-03T01:17:16.027270+00:00","updated_at":"2026-07-03T01:17:16.027270+00:00"}