{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:TI2ZUIAOWBQWLGSFIEC4LRSRIB","short_pith_number":"pith:TI2ZUIAO","schema_version":"1.0","canonical_sha256":"9a359a200eb061659a454105c5c6514061082e2db1915072c42b8642f38b2a8e","source":{"kind":"arxiv","id":"2409.02807","version":4},"attestation_state":"computed","paper":{"title":"Primordial regular black holes as all the dark matter. II. Non-time-radial-symmetric and loop quantum gravity-inspired metrics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Davide Pedrotti, Marco Calz\\`a, Sunny Vagnozzi","submitted_at":"2024-09-04T15:25:06Z","abstract_excerpt":"It is a common belief that a theory of quantum gravity should ultimately cure curvature singularities which are inevitable within General Relativity, and plague for instance the Schwarzschild and Kerr metrics, usually considered as prototypes for primordial black holes (PBHs) as dark matter (DM) candidates. We continue our study, initiated in a companion paper, of non-singular objects as PBHs, considering three regular non-tr (non-time-radial)-symmetric metrics, all of which are one-parameter extensions of the Schwarzschild space-time: the Simpson-Visser, Peltola-Kunstatter, and D'Ambrosio-Rov"},"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":"2409.02807","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2024-09-04T15:25:06Z","cross_cats_sorted":["astro-ph.CO","hep-ph","hep-th"],"title_canon_sha256":"be90ca9c45e9951cb66b01261bcee3e274439d758950780761c80e32e6c296f3","abstract_canon_sha256":"649ea4af0d6a91b733069e4f45572c288f4f7ffd106acb9efa9698278f257246"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:07:26.866800Z","signature_b64":"J3JO5P/E9GgX0ksXHd5RusvlxTSmUdjzNZtX+ptGRmJw/0gdFUh77qrvfbiEEfc8mI/k355mCp76sRBcz31rDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9a359a200eb061659a454105c5c6514061082e2db1915072c42b8642f38b2a8e","last_reissued_at":"2026-07-05T10:07:26.866264Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:07:26.866264Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Primordial regular black holes as all the dark matter. II. Non-time-radial-symmetric and loop quantum gravity-inspired metrics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Davide Pedrotti, Marco Calz\\`a, Sunny Vagnozzi","submitted_at":"2024-09-04T15:25:06Z","abstract_excerpt":"It is a common belief that a theory of quantum gravity should ultimately cure curvature singularities which are inevitable within General Relativity, and plague for instance the Schwarzschild and Kerr metrics, usually considered as prototypes for primordial black holes (PBHs) as dark matter (DM) candidates. We continue our study, initiated in a companion paper, of non-singular objects as PBHs, considering three regular non-tr (non-time-radial)-symmetric metrics, all of which are one-parameter extensions of the Schwarzschild space-time: the Simpson-Visser, Peltola-Kunstatter, and D'Ambrosio-Rov"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2409.02807","kind":"arxiv","version":4},"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/2409.02807/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":"2409.02807","created_at":"2026-07-05T10:07:26.866345+00:00"},{"alias_kind":"arxiv_version","alias_value":"2409.02807v4","created_at":"2026-07-05T10:07:26.866345+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2409.02807","created_at":"2026-07-05T10:07:26.866345+00:00"},{"alias_kind":"pith_short_12","alias_value":"TI2ZUIAOWBQW","created_at":"2026-07-05T10:07:26.866345+00:00"},{"alias_kind":"pith_short_16","alias_value":"TI2ZUIAOWBQWLGSF","created_at":"2026-07-05T10:07:26.866345+00:00"},{"alias_kind":"pith_short_8","alias_value":"TI2ZUIAO","created_at":"2026-07-05T10:07:26.866345+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":10,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07011","citing_title":"Primordial black hole in Lorentz-violating theories: Insights from Bumblebee gravity","ref_index":44,"is_internal_anchor":true},{"citing_arxiv_id":"2606.09983","citing_title":"Anomaly-driven evaporation endpoints of a two-dimensional regular black hole","ref_index":33,"is_internal_anchor":false},{"citing_arxiv_id":"2606.06355","citing_title":"$\\tt BlackHawk$ $\\tt v3.0$: Hawking Radiation from Regular Black Holes","ref_index":243,"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":31,"is_internal_anchor":false},{"citing_arxiv_id":"2510.09395","citing_title":"Dark matter production from evaporation of regular primordial black holes","ref_index":65,"is_internal_anchor":false},{"citing_arxiv_id":"2605.19463","citing_title":"Memory burden effect of regular primordial black holes","ref_index":93,"is_internal_anchor":false},{"citing_arxiv_id":"2509.13335","citing_title":"Regular black holes with gravitational self-energy as dark matter","ref_index":22,"is_internal_anchor":false},{"citing_arxiv_id":"2601.10806","citing_title":"Shadow signatures and energy accumulation in Lorentzian-Euclidean black holes","ref_index":44,"is_internal_anchor":false},{"citing_arxiv_id":"2603.25084","citing_title":"Particle motions and gravitational waveforms in rotating black hole spacetimes of loop quantum gravity","ref_index":69,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05232","citing_title":"Inflation driven by repulsive-like primordial black holes","ref_index":45,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TI2ZUIAOWBQWLGSFIEC4LRSRIB","json":"https://pith.science/pith/TI2ZUIAOWBQWLGSFIEC4LRSRIB.json","graph_json":"https://pith.science/api/pith-number/TI2ZUIAOWBQWLGSFIEC4LRSRIB/graph.json","events_json":"https://pith.science/api/pith-number/TI2ZUIAOWBQWLGSFIEC4LRSRIB/events.json","paper":"https://pith.science/paper/TI2ZUIAO"},"agent_actions":{"view_html":"https://pith.science/pith/TI2ZUIAOWBQWLGSFIEC4LRSRIB","download_json":"https://pith.science/pith/TI2ZUIAOWBQWLGSFIEC4LRSRIB.json","view_paper":"https://pith.science/paper/TI2ZUIAO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2409.02807&json=true","fetch_graph":"https://pith.science/api/pith-number/TI2ZUIAOWBQWLGSFIEC4LRSRIB/graph.json","fetch_events":"https://pith.science/api/pith-number/TI2ZUIAOWBQWLGSFIEC4LRSRIB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TI2ZUIAOWBQWLGSFIEC4LRSRIB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TI2ZUIAOWBQWLGSFIEC4LRSRIB/action/storage_attestation","attest_author":"https://pith.science/pith/TI2ZUIAOWBQWLGSFIEC4LRSRIB/action/author_attestation","sign_citation":"https://pith.science/pith/TI2ZUIAOWBQWLGSFIEC4LRSRIB/action/citation_signature","submit_replication":"https://pith.science/pith/TI2ZUIAOWBQWLGSFIEC4LRSRIB/action/replication_record"}},"created_at":"2026-07-05T10:07:26.866345+00:00","updated_at":"2026-07-05T10:07:26.866345+00:00"}