{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:4YFFGE4DT5T4D2XNC7RJHCHJRM","short_pith_number":"pith:4YFFGE4D","schema_version":"1.0","canonical_sha256":"e60a5313839f67c1eaed17e29388e98b3474f3f14de4dddf2f9d4e6c1dbc5d8e","source":{"kind":"arxiv","id":"2405.00124","version":2},"attestation_state":"computed","paper":{"title":"Primordial black hole probes of heavy neutral leptons","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Agnese Tolino, Valentina De Romeri, Yuber F. Perez-Gonzalez","submitted_at":"2024-04-30T18:17:47Z","abstract_excerpt":"Primordial black holes (PBH), while still constituting a viable dark matter component, are expected to evaporate through Hawking radiation. Assuming the semi-classical approximation holds up to near the Planck scale, PBHs are expected to evaporate by the present time, emitting a significant flux of particles in their final moments, if produced in the early Universe with an initial mass of $\\sim 10^{15}$ g. These ``exploding'' black holes will release a burst of Standard Model particles alongside any additional degrees of freedom, should they exist. We explore the possibility that heavy neutral"},"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":"2405.00124","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2024-04-30T18:17:47Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"98ad56d654af523c35bdd2de4ece077c81f627ad9947bee90db13ff86375f8e7","abstract_canon_sha256":"c9fed0f715477c11f69ba9da394ef8ad5ea1fc7f16ff09aa10498d20d4c4d575"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:28:04.687370Z","signature_b64":"SnhHTZUGiIyKTVL8NI82WZZaNBztetGqYikbrKloMQgzDOSzQWYnugHXqEqFxs9IUhKafjTos7cmRGdMHIYOCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e60a5313839f67c1eaed17e29388e98b3474f3f14de4dddf2f9d4e6c1dbc5d8e","last_reissued_at":"2026-07-05T10:28:04.686868Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:28:04.686868Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Primordial black hole probes of heavy neutral leptons","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Agnese Tolino, Valentina De Romeri, Yuber F. Perez-Gonzalez","submitted_at":"2024-04-30T18:17:47Z","abstract_excerpt":"Primordial black holes (PBH), while still constituting a viable dark matter component, are expected to evaporate through Hawking radiation. Assuming the semi-classical approximation holds up to near the Planck scale, PBHs are expected to evaporate by the present time, emitting a significant flux of particles in their final moments, if produced in the early Universe with an initial mass of $\\sim 10^{15}$ g. These ``exploding'' black holes will release a burst of Standard Model particles alongside any additional degrees of freedom, should they exist. We explore the possibility that heavy neutral"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.00124","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/2405.00124/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":"2405.00124","created_at":"2026-07-05T10:28:04.686926+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.00124v2","created_at":"2026-07-05T10:28:04.686926+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.00124","created_at":"2026-07-05T10:28:04.686926+00:00"},{"alias_kind":"pith_short_12","alias_value":"4YFFGE4DT5T4","created_at":"2026-07-05T10:28:04.686926+00:00"},{"alias_kind":"pith_short_16","alias_value":"4YFFGE4DT5T4D2XN","created_at":"2026-07-05T10:28:04.686926+00:00"},{"alias_kind":"pith_short_8","alias_value":"4YFFGE4D","created_at":"2026-07-05T10:28:04.686926+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.06355","citing_title":"$\\tt BlackHawk$ $\\tt v3.0$: Hawking Radiation from Regular Black Holes","ref_index":231,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4YFFGE4DT5T4D2XNC7RJHCHJRM","json":"https://pith.science/pith/4YFFGE4DT5T4D2XNC7RJHCHJRM.json","graph_json":"https://pith.science/api/pith-number/4YFFGE4DT5T4D2XNC7RJHCHJRM/graph.json","events_json":"https://pith.science/api/pith-number/4YFFGE4DT5T4D2XNC7RJHCHJRM/events.json","paper":"https://pith.science/paper/4YFFGE4D"},"agent_actions":{"view_html":"https://pith.science/pith/4YFFGE4DT5T4D2XNC7RJHCHJRM","download_json":"https://pith.science/pith/4YFFGE4DT5T4D2XNC7RJHCHJRM.json","view_paper":"https://pith.science/paper/4YFFGE4D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.00124&json=true","fetch_graph":"https://pith.science/api/pith-number/4YFFGE4DT5T4D2XNC7RJHCHJRM/graph.json","fetch_events":"https://pith.science/api/pith-number/4YFFGE4DT5T4D2XNC7RJHCHJRM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4YFFGE4DT5T4D2XNC7RJHCHJRM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4YFFGE4DT5T4D2XNC7RJHCHJRM/action/storage_attestation","attest_author":"https://pith.science/pith/4YFFGE4DT5T4D2XNC7RJHCHJRM/action/author_attestation","sign_citation":"https://pith.science/pith/4YFFGE4DT5T4D2XNC7RJHCHJRM/action/citation_signature","submit_replication":"https://pith.science/pith/4YFFGE4DT5T4D2XNC7RJHCHJRM/action/replication_record"}},"created_at":"2026-07-05T10:28:04.686926+00:00","updated_at":"2026-07-05T10:28:04.686926+00:00"}