{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:OSCPBELOYVJBRGRDPHTNBMNN6O","short_pith_number":"pith:OSCPBELO","schema_version":"1.0","canonical_sha256":"7484f0916ec552189a2379e6d0b1adf38e43d9744383919322d7246500cdac35","source":{"kind":"arxiv","id":"2501.05505","version":2},"attestation_state":"computed","paper":{"title":"Towards a Non-singular Paradigm of Black Hole Physics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Alessia Platania, Alfio Bonanno, Antonio Panassiti, Astrid Eichhorn, Carlos Barcel\\'o, Daniel Jampolski, Francesco Del Porro, Francesco Di Filippo, Jacopo Mazza, Johanna Borissova, Julio Arrechea, Luciano Rezzolla, Matt Visser, Paolo Pani, Prado Mart\\'in-Moruno, Ra\\'ul Carballo-Rubio, Stefano Liberati, Tyler McMaken, Valentin Boyanov, Vania Vellucci, Vitor Cardoso","submitted_at":"2025-01-09T19:00:00Z","abstract_excerpt":"The study of regular black holes and black hole mimickers as alternatives to standard black holes has recently gained significant attention, driven both by the need to extend general relativity to describe black hole interiors, and by recent advances in observational technologies. Despite considerable progress in this field, significant challenges remain in identifying and characterizing physically well-motivated classes of regular black holes and black hole mimickers. This report provides an overview of these challenges, and outlines some of the promising research directions -- as discussed d"},"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":"2501.05505","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2025-01-09T19:00:00Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"dc01c3f47feeae78da57f8638a30ac7e93312cfbeccf7b47e6f1cc2f1cfcb825","abstract_canon_sha256":"5839115d946ab794c4cc2367b1a0f95f81dc250e8beb796f05e93d4c0ee7677e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:14:01.928098Z","signature_b64":"bXsx5WAiikDcu0CSJZ3LdUDghYt/nJo7ibReXjwjhL7NfsbQe10uB6CjWs3/3pIFmYVG238+pBqaHDQPAnGFBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7484f0916ec552189a2379e6d0b1adf38e43d9744383919322d7246500cdac35","last_reissued_at":"2026-07-05T11:14:01.927610Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:14:01.927610Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Towards a Non-singular Paradigm of Black Hole Physics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Alessia Platania, Alfio Bonanno, Antonio Panassiti, Astrid Eichhorn, Carlos Barcel\\'o, Daniel Jampolski, Francesco Del Porro, Francesco Di Filippo, Jacopo Mazza, Johanna Borissova, Julio Arrechea, Luciano Rezzolla, Matt Visser, Paolo Pani, Prado Mart\\'in-Moruno, Ra\\'ul Carballo-Rubio, Stefano Liberati, Tyler McMaken, Valentin Boyanov, Vania Vellucci, Vitor Cardoso","submitted_at":"2025-01-09T19:00:00Z","abstract_excerpt":"The study of regular black holes and black hole mimickers as alternatives to standard black holes has recently gained significant attention, driven both by the need to extend general relativity to describe black hole interiors, and by recent advances in observational technologies. Despite considerable progress in this field, significant challenges remain in identifying and characterizing physically well-motivated classes of regular black holes and black hole mimickers. This report provides an overview of these challenges, and outlines some of the promising research directions -- as discussed d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2501.05505","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/2501.05505/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":"2501.05505","created_at":"2026-07-05T11:14:01.927668+00:00"},{"alias_kind":"arxiv_version","alias_value":"2501.05505v2","created_at":"2026-07-05T11:14:01.927668+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2501.05505","created_at":"2026-07-05T11:14:01.927668+00:00"},{"alias_kind":"pith_short_12","alias_value":"OSCPBELOYVJB","created_at":"2026-07-05T11:14:01.927668+00:00"},{"alias_kind":"pith_short_16","alias_value":"OSCPBELOYVJBRGRD","created_at":"2026-07-05T11:14:01.927668+00:00"},{"alias_kind":"pith_short_8","alias_value":"OSCPBELO","created_at":"2026-07-05T11:14:01.927668+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":21,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2607.07790","citing_title":"Regular Black Holes in Nonlocal Quasitopological Gravity","ref_index":84,"is_internal_anchor":true},{"citing_arxiv_id":"2607.07831","citing_title":"Charging up regular black holes","ref_index":4,"is_internal_anchor":true},{"citing_arxiv_id":"2606.22404","citing_title":"Null geodesic defocusing in dynamical black-hole-to-white-hole transitions","ref_index":7,"is_internal_anchor":false},{"citing_arxiv_id":"2605.30340","citing_title":"Carr criterion and mass gaps in non-singular primordial black hole formation","ref_index":54,"is_internal_anchor":false},{"citing_arxiv_id":"2605.15576","citing_title":"Regular black hole with sub-Planckian curvature and suppressed exponential mass inflation","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2506.14875","citing_title":"Regular Vaidya solutions of effective gravitational theories","ref_index":17,"is_internal_anchor":false},{"citing_arxiv_id":"2510.07467","citing_title":"Weakly turbulent saturation of the nonlinear scalar ergoregion instability","ref_index":42,"is_internal_anchor":false},{"citing_arxiv_id":"2510.20649","citing_title":"Radiating black holes in general relativity need not be singular","ref_index":6,"is_internal_anchor":false},{"citing_arxiv_id":"2511.10307","citing_title":"Gravitational Atoms from Topological Stars","ref_index":10,"is_internal_anchor":false},{"citing_arxiv_id":"2601.17115","citing_title":"Effective geometrodynamics for renormalization-group improved black-hole spacetimes in spherical symmetry","ref_index":2,"is_internal_anchor":false},{"citing_arxiv_id":"2603.06786","citing_title":"All $2D$ generalised dilaton theories from $d\\geq 4$ gravities","ref_index":147,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26191","citing_title":"Gravitational Properties of the Monopole Bag","ref_index":88,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03428","citing_title":"Families of regular spacetimes and energy conditions","ref_index":16,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26191","citing_title":"Gravitational Properties of the Monopole Bag","ref_index":88,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03428","citing_title":"Families of regular spacetimes and energy conditions","ref_index":16,"is_internal_anchor":false},{"citing_arxiv_id":"2604.24101","citing_title":"$g_{tt}g_{rr} =-1$ black hole thermodynamics in extended quasi-topological gravity","ref_index":111,"is_internal_anchor":false},{"citing_arxiv_id":"2605.06813","citing_title":"Towards black-hole horizons and geodesic focusing in causal sets","ref_index":68,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18004","citing_title":"Eikonal, nonlocality and regular black holes","ref_index":36,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15260","citing_title":"Taming the Aretakis instability: extremal black holes with multi-degenerate horizons","ref_index":4,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15758","citing_title":"Geometrically Regular Black Holes with Hedgehog Scalar Hair","ref_index":2,"is_internal_anchor":false},{"citing_arxiv_id":"2604.16545","citing_title":"Energy conditions in static, spherically symmetric spacetimes and effective geometries","ref_index":34,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OSCPBELOYVJBRGRDPHTNBMNN6O","json":"https://pith.science/pith/OSCPBELOYVJBRGRDPHTNBMNN6O.json","graph_json":"https://pith.science/api/pith-number/OSCPBELOYVJBRGRDPHTNBMNN6O/graph.json","events_json":"https://pith.science/api/pith-number/OSCPBELOYVJBRGRDPHTNBMNN6O/events.json","paper":"https://pith.science/paper/OSCPBELO"},"agent_actions":{"view_html":"https://pith.science/pith/OSCPBELOYVJBRGRDPHTNBMNN6O","download_json":"https://pith.science/pith/OSCPBELOYVJBRGRDPHTNBMNN6O.json","view_paper":"https://pith.science/paper/OSCPBELO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2501.05505&json=true","fetch_graph":"https://pith.science/api/pith-number/OSCPBELOYVJBRGRDPHTNBMNN6O/graph.json","fetch_events":"https://pith.science/api/pith-number/OSCPBELOYVJBRGRDPHTNBMNN6O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OSCPBELOYVJBRGRDPHTNBMNN6O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OSCPBELOYVJBRGRDPHTNBMNN6O/action/storage_attestation","attest_author":"https://pith.science/pith/OSCPBELOYVJBRGRDPHTNBMNN6O/action/author_attestation","sign_citation":"https://pith.science/pith/OSCPBELOYVJBRGRDPHTNBMNN6O/action/citation_signature","submit_replication":"https://pith.science/pith/OSCPBELOYVJBRGRDPHTNBMNN6O/action/replication_record"}},"created_at":"2026-07-05T11:14:01.927668+00:00","updated_at":"2026-07-05T11:14:01.927668+00:00"}