{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:C7IA57FLSHL4CTY4SGOL4L4OUL","short_pith_number":"pith:C7IA57FL","schema_version":"1.0","canonical_sha256":"17d00efcab91d7c14f1c919cbe2f8ea2fd9e5c4f9f1db515e13aefb6a6a991e5","source":{"kind":"arxiv","id":"2105.06504","version":2},"attestation_state":"computed","paper":{"title":"Neutron Star Quantum Death by Small Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","astro-ph.SR","gr-qc"],"primary_cat":"hep-ph","authors_text":"John Lloyd, Pierce Giffin, Samuel D. McDermott, Stefano Profumo","submitted_at":"2021-05-13T18:34:38Z","abstract_excerpt":"Neutron stars can be destroyed by black holes at their center accreting material and eventually swallowing the entire star. Here we note that the accretion model adopted in the literature, based on Bondi accretion or variations thereof, is inadequate for small black holes -- black holes whose Schwarzschild radius is comparable to, or smaller than, the neutron's de Broglie wavelength. In this case, quantum mechanical aspects of the accretion process cannot be neglected, and give rise to a completely different accretion rate. We show that for the case of black holes seeded by the collapse of bos"},"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":"2105.06504","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2021-05-13T18:34:38Z","cross_cats_sorted":["astro-ph.HE","astro-ph.SR","gr-qc"],"title_canon_sha256":"a7691b6eaca1f36130834221bc282db1180b8ee3609d96bb409d1bac8b95f454","abstract_canon_sha256":"d3278ca504af8590b8990152ac3e13f9d557f4ba69a883889d09e4be46bd0421"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:34:25.883802Z","signature_b64":"uROq1QitEFAKR9ka/WDB/uyHa91xTs6JYgTRmSoBP7L+MhH9BjGZITrAG6ROR7BL3gY3LoQ9QQlZzsU+LVfYDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"17d00efcab91d7c14f1c919cbe2f8ea2fd9e5c4f9f1db515e13aefb6a6a991e5","last_reissued_at":"2026-07-05T04:34:25.883323Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:34:25.883323Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutron Star Quantum Death by Small Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","astro-ph.SR","gr-qc"],"primary_cat":"hep-ph","authors_text":"John Lloyd, Pierce Giffin, Samuel D. McDermott, Stefano Profumo","submitted_at":"2021-05-13T18:34:38Z","abstract_excerpt":"Neutron stars can be destroyed by black holes at their center accreting material and eventually swallowing the entire star. Here we note that the accretion model adopted in the literature, based on Bondi accretion or variations thereof, is inadequate for small black holes -- black holes whose Schwarzschild radius is comparable to, or smaller than, the neutron's de Broglie wavelength. In this case, quantum mechanical aspects of the accretion process cannot be neglected, and give rise to a completely different accretion rate. We show that for the case of black holes seeded by the collapse of bos"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2105.06504","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/2105.06504/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":"2105.06504","created_at":"2026-07-05T04:34:25.883386+00:00"},{"alias_kind":"arxiv_version","alias_value":"2105.06504v2","created_at":"2026-07-05T04:34:25.883386+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2105.06504","created_at":"2026-07-05T04:34:25.883386+00:00"},{"alias_kind":"pith_short_12","alias_value":"C7IA57FLSHL4","created_at":"2026-07-05T04:34:25.883386+00:00"},{"alias_kind":"pith_short_16","alias_value":"C7IA57FLSHL4CTY4","created_at":"2026-07-05T04:34:25.883386+00:00"},{"alias_kind":"pith_short_8","alias_value":"C7IA57FL","created_at":"2026-07-05T04:34:25.883386+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/C7IA57FLSHL4CTY4SGOL4L4OUL","json":"https://pith.science/pith/C7IA57FLSHL4CTY4SGOL4L4OUL.json","graph_json":"https://pith.science/api/pith-number/C7IA57FLSHL4CTY4SGOL4L4OUL/graph.json","events_json":"https://pith.science/api/pith-number/C7IA57FLSHL4CTY4SGOL4L4OUL/events.json","paper":"https://pith.science/paper/C7IA57FL"},"agent_actions":{"view_html":"https://pith.science/pith/C7IA57FLSHL4CTY4SGOL4L4OUL","download_json":"https://pith.science/pith/C7IA57FLSHL4CTY4SGOL4L4OUL.json","view_paper":"https://pith.science/paper/C7IA57FL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2105.06504&json=true","fetch_graph":"https://pith.science/api/pith-number/C7IA57FLSHL4CTY4SGOL4L4OUL/graph.json","fetch_events":"https://pith.science/api/pith-number/C7IA57FLSHL4CTY4SGOL4L4OUL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/C7IA57FLSHL4CTY4SGOL4L4OUL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/C7IA57FLSHL4CTY4SGOL4L4OUL/action/storage_attestation","attest_author":"https://pith.science/pith/C7IA57FLSHL4CTY4SGOL4L4OUL/action/author_attestation","sign_citation":"https://pith.science/pith/C7IA57FLSHL4CTY4SGOL4L4OUL/action/citation_signature","submit_replication":"https://pith.science/pith/C7IA57FLSHL4CTY4SGOL4L4OUL/action/replication_record"}},"created_at":"2026-07-05T04:34:25.883386+00:00","updated_at":"2026-07-05T04:34:25.883386+00:00"}