{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:OVSIIPJOFUNA3XJ3LHKYWM7RQ4","short_pith_number":"pith:OVSIIPJO","schema_version":"1.0","canonical_sha256":"7564843d2e2d1a0ddd3b59d58b33f187135d78e95038fd639c5a00897f4f9d9b","source":{"kind":"arxiv","id":"2402.15211","version":1},"attestation_state":"computed","paper":{"title":"Primordial Black Holes as a dark matter candidate -- a brief overview","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Anne M. Green","submitted_at":"2024-02-23T09:16:57Z","abstract_excerpt":"Historically the most popular dark matter candidates have been new elementary particles, such as Weakly Interacting Massive Particles and axions. However Primordial Black Holes (PBHs), black holes formed from overdensities in the early Universe, are another possibility. The discovery of gravitational waves from mergers of tens of Solar mass black hole binaries by LIGO-Virgo has generated a surge in interest in PBH dark matter. We overview the formation of PBHs, observational probes of their abundance, and some of the key open questions in the field."},"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":"2402.15211","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-02-23T09:16:57Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"e698be7ad7eaa203fcce9ad115f227a7f6886dfaf0bb8997c9c489d1d503b6f8","abstract_canon_sha256":"7256294051028ef2e6bfd29798e2ac1adc87e69c2db4730d192454ba46e8f5f9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:48:37.406863Z","signature_b64":"itfVTa53fG2Q4f+AfPBqctc9jojRiwM+Fc4duCGkLNAeShxnWme3wZpIgPpRZZKwtfnrCg6L/voZu5I4yn/sBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7564843d2e2d1a0ddd3b59d58b33f187135d78e95038fd639c5a00897f4f9d9b","last_reissued_at":"2026-07-05T07:48:37.406394Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:48:37.406394Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Primordial Black Holes as a dark matter candidate -- a brief overview","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Anne M. Green","submitted_at":"2024-02-23T09:16:57Z","abstract_excerpt":"Historically the most popular dark matter candidates have been new elementary particles, such as Weakly Interacting Massive Particles and axions. However Primordial Black Holes (PBHs), black holes formed from overdensities in the early Universe, are another possibility. The discovery of gravitational waves from mergers of tens of Solar mass black hole binaries by LIGO-Virgo has generated a surge in interest in PBH dark matter. We overview the formation of PBHs, observational probes of their abundance, and some of the key open questions in the field."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2402.15211","kind":"arxiv","version":1},"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/2402.15211/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":"2402.15211","created_at":"2026-07-05T07:48:37.406454+00:00"},{"alias_kind":"arxiv_version","alias_value":"2402.15211v1","created_at":"2026-07-05T07:48:37.406454+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2402.15211","created_at":"2026-07-05T07:48:37.406454+00:00"},{"alias_kind":"pith_short_12","alias_value":"OVSIIPJOFUNA","created_at":"2026-07-05T07:48:37.406454+00:00"},{"alias_kind":"pith_short_16","alias_value":"OVSIIPJOFUNA3XJ3","created_at":"2026-07-05T07:48:37.406454+00:00"},{"alias_kind":"pith_short_8","alias_value":"OVSIIPJO","created_at":"2026-07-05T07:48:37.406454+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2505.00563","citing_title":"Dark matter and modified gravity: Einstein clusters from a non-minimally coupled vector field","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2605.19463","citing_title":"Memory burden effect of regular primordial black holes","ref_index":24,"is_internal_anchor":false},{"citing_arxiv_id":"2510.11861","citing_title":"Impact of facility timing and coordination for next-generation gravitational-wave detectors","ref_index":34,"is_internal_anchor":false},{"citing_arxiv_id":"2603.18884","citing_title":"Primordial black holes and the velocity acoustic oscillations features in 21 cm signals from the cosmic Dark Ages","ref_index":89,"is_internal_anchor":false},{"citing_arxiv_id":"2604.24654","citing_title":"SWIM: Stochastic Warm Inflation Module to generate and analyse Warm Inflationary power spectrum","ref_index":26,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OVSIIPJOFUNA3XJ3LHKYWM7RQ4","json":"https://pith.science/pith/OVSIIPJOFUNA3XJ3LHKYWM7RQ4.json","graph_json":"https://pith.science/api/pith-number/OVSIIPJOFUNA3XJ3LHKYWM7RQ4/graph.json","events_json":"https://pith.science/api/pith-number/OVSIIPJOFUNA3XJ3LHKYWM7RQ4/events.json","paper":"https://pith.science/paper/OVSIIPJO"},"agent_actions":{"view_html":"https://pith.science/pith/OVSIIPJOFUNA3XJ3LHKYWM7RQ4","download_json":"https://pith.science/pith/OVSIIPJOFUNA3XJ3LHKYWM7RQ4.json","view_paper":"https://pith.science/paper/OVSIIPJO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2402.15211&json=true","fetch_graph":"https://pith.science/api/pith-number/OVSIIPJOFUNA3XJ3LHKYWM7RQ4/graph.json","fetch_events":"https://pith.science/api/pith-number/OVSIIPJOFUNA3XJ3LHKYWM7RQ4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OVSIIPJOFUNA3XJ3LHKYWM7RQ4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OVSIIPJOFUNA3XJ3LHKYWM7RQ4/action/storage_attestation","attest_author":"https://pith.science/pith/OVSIIPJOFUNA3XJ3LHKYWM7RQ4/action/author_attestation","sign_citation":"https://pith.science/pith/OVSIIPJOFUNA3XJ3LHKYWM7RQ4/action/citation_signature","submit_replication":"https://pith.science/pith/OVSIIPJOFUNA3XJ3LHKYWM7RQ4/action/replication_record"}},"created_at":"2026-07-05T07:48:37.406454+00:00","updated_at":"2026-07-05T07:48:37.406454+00:00"}