{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:PARTCVFJFKJATBJMMO45DZR4CT","short_pith_number":"pith:PARTCVFJ","schema_version":"1.0","canonical_sha256":"78233154a92a9209852c63b9d1e63c14c12e5e3620019a5a50655d8c6a158408","source":{"kind":"arxiv","id":"2501.16134","version":3},"attestation_state":"computed","paper":{"title":"Quasinormal Ringing and Shadows of Black Holes and Wormholes in Dark Matter-Inspired Weyl Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Alexander Zhidenko, Andrii Khrabustovskyi, Jan K\\v{r}\\'i\\v{z}, Roman A. Konoplya","submitted_at":"2025-01-27T15:24:58Z","abstract_excerpt":"Weyl gravity naturally generates effective dark matter and cosmological constant terms as integration constants, eliminating the need to explicitly introduce them into the theory. Additionally, the framework permits three intriguing solutions for compact objects: an asymptotically de Sitter Schwarzschild-like black hole described by the Mannheim-Kazanas solution, a non-Schwarzschild black hole, and a traversable wormhole that exists without exotic matter. In this work, we investigate the quasinormal spectra of all three solutions.\n  We demonstrate that when the mass of the black hole correspon"},"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":"2501.16134","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2025-01-27T15:24:58Z","cross_cats_sorted":[],"title_canon_sha256":"db1bb3b07c6d84019080c35f480911e378de110e7cb078c09e9640e2f5428d00","abstract_canon_sha256":"a3968fa1fd3cfbb214ce77a0301498b0b767ba96cd8117671abb666b9d0070e2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:53:15.354741Z","signature_b64":"AxLkIxpi/W4B0fgtHVNswkGEPE0hKr7YfDSsrWg6OShIPISawOVh70DCa8iJ/h1kq62mhjSjbopFqrObEFSKAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"78233154a92a9209852c63b9d1e63c14c12e5e3620019a5a50655d8c6a158408","last_reissued_at":"2026-07-05T10:53:15.354230Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:53:15.354230Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quasinormal Ringing and Shadows of Black Holes and Wormholes in Dark Matter-Inspired Weyl Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Alexander Zhidenko, Andrii Khrabustovskyi, Jan K\\v{r}\\'i\\v{z}, Roman A. Konoplya","submitted_at":"2025-01-27T15:24:58Z","abstract_excerpt":"Weyl gravity naturally generates effective dark matter and cosmological constant terms as integration constants, eliminating the need to explicitly introduce them into the theory. Additionally, the framework permits three intriguing solutions for compact objects: an asymptotically de Sitter Schwarzschild-like black hole described by the Mannheim-Kazanas solution, a non-Schwarzschild black hole, and a traversable wormhole that exists without exotic matter. In this work, we investigate the quasinormal spectra of all three solutions.\n  We demonstrate that when the mass of the black hole correspon"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2501.16134","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/2501.16134/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":"2501.16134","created_at":"2026-07-05T10:53:15.354288+00:00"},{"alias_kind":"arxiv_version","alias_value":"2501.16134v3","created_at":"2026-07-05T10:53:15.354288+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2501.16134","created_at":"2026-07-05T10:53:15.354288+00:00"},{"alias_kind":"pith_short_12","alias_value":"PARTCVFJFKJA","created_at":"2026-07-05T10:53:15.354288+00:00"},{"alias_kind":"pith_short_16","alias_value":"PARTCVFJFKJATBJM","created_at":"2026-07-05T10:53:15.354288+00:00"},{"alias_kind":"pith_short_8","alias_value":"PARTCVFJ","created_at":"2026-07-05T10:53:15.354288+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2508.00203","citing_title":"Quantum-Corrected Thermodynamics of Conformal Weyl Gravity Black Holes: GUP Effects and Phase Transitions","ref_index":66,"is_internal_anchor":false},{"citing_arxiv_id":"2512.23510","citing_title":"Quasinormal mode/grey-body factor correspondence for Kerr black holes","ref_index":42,"is_internal_anchor":false},{"citing_arxiv_id":"2601.18613","citing_title":"Correspondence between quasinormal modes and grey-body factors of Schwarzschild--Tangherlini black holes","ref_index":80,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14999","citing_title":"A First-Order Eikonal Framework for Quasinormal Modes, Shadows, Strong Lensing, and Grey-Body Factors in a Scalarized Black-Hole Metric","ref_index":38,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14999","citing_title":"A First-Order Eikonal Framework for Quasinormal Modes, Shadows, Strong Lensing, and Grey-Body Factors in a Scalarized Black-Hole Metric","ref_index":38,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PARTCVFJFKJATBJMMO45DZR4CT","json":"https://pith.science/pith/PARTCVFJFKJATBJMMO45DZR4CT.json","graph_json":"https://pith.science/api/pith-number/PARTCVFJFKJATBJMMO45DZR4CT/graph.json","events_json":"https://pith.science/api/pith-number/PARTCVFJFKJATBJMMO45DZR4CT/events.json","paper":"https://pith.science/paper/PARTCVFJ"},"agent_actions":{"view_html":"https://pith.science/pith/PARTCVFJFKJATBJMMO45DZR4CT","download_json":"https://pith.science/pith/PARTCVFJFKJATBJMMO45DZR4CT.json","view_paper":"https://pith.science/paper/PARTCVFJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2501.16134&json=true","fetch_graph":"https://pith.science/api/pith-number/PARTCVFJFKJATBJMMO45DZR4CT/graph.json","fetch_events":"https://pith.science/api/pith-number/PARTCVFJFKJATBJMMO45DZR4CT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PARTCVFJFKJATBJMMO45DZR4CT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PARTCVFJFKJATBJMMO45DZR4CT/action/storage_attestation","attest_author":"https://pith.science/pith/PARTCVFJFKJATBJMMO45DZR4CT/action/author_attestation","sign_citation":"https://pith.science/pith/PARTCVFJFKJATBJMMO45DZR4CT/action/citation_signature","submit_replication":"https://pith.science/pith/PARTCVFJFKJATBJMMO45DZR4CT/action/replication_record"}},"created_at":"2026-07-05T10:53:15.354288+00:00","updated_at":"2026-07-05T10:53:15.354288+00:00"}