{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:AH5CDLSWLOEPGJMQ53HEHYXPYF","short_pith_number":"pith:AH5CDLSW","schema_version":"1.0","canonical_sha256":"01fa21ae565b88f32590eece43e2efc17428b942186e57534d3bfac09376a784","source":{"kind":"arxiv","id":"1709.07467","version":2},"attestation_state":"computed","paper":{"title":"Primordial Black Holes as Dark Matter: Converting Constraints from Monochromatic to Extended Mass Distributions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alvise Raccanelli, Jos\\'e Luis Bernal, Licia Verde, Nicola Bellomo","submitted_at":"2017-09-21T18:10:39Z","abstract_excerpt":"The model in which Primordial Black Holes (PBHs) constitute a non-negligible fraction of the dark matter has (re)gained popularity after the first detections of binary black hole mergers. Most of the observational constraints to date have been derived assuming a single mass for all the PBHs, although some more recent works tried to generalize constraints to the case of extended mass functions. Here we derive a general methodology to obtain constraints for any PBH Extended Mass Distribution (EMD) and any observables in the desired mass range. Starting from those obtained for a monochromatic dis"},"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":"1709.07467","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-09-21T18:10:39Z","cross_cats_sorted":[],"title_canon_sha256":"b43a93472b38ce3c7d80a7e2eb9f5ef4f00ea0acee3accc56aecd780ee5bcbb8","abstract_canon_sha256":"363fa5b9b630042869a605d699fc3e489312135a49006975cab2c87213e86c0d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:26:19.141988Z","signature_b64":"L0trBkCpHc2DAm3xnCPUO6HgWpajdNQriZGra6XETrft0RiHmuwdTJmdT/eE2vf5sgpRSE+LrF3Jpo6yYeoHCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"01fa21ae565b88f32590eece43e2efc17428b942186e57534d3bfac09376a784","last_reissued_at":"2026-05-18T00:26:19.141369Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:26:19.141369Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Primordial Black Holes as Dark Matter: Converting Constraints from Monochromatic to Extended Mass Distributions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alvise Raccanelli, Jos\\'e Luis Bernal, Licia Verde, Nicola Bellomo","submitted_at":"2017-09-21T18:10:39Z","abstract_excerpt":"The model in which Primordial Black Holes (PBHs) constitute a non-negligible fraction of the dark matter has (re)gained popularity after the first detections of binary black hole mergers. Most of the observational constraints to date have been derived assuming a single mass for all the PBHs, although some more recent works tried to generalize constraints to the case of extended mass functions. Here we derive a general methodology to obtain constraints for any PBH Extended Mass Distribution (EMD) and any observables in the desired mass range. Starting from those obtained for a monochromatic dis"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.07467","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":""},"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":"1709.07467","created_at":"2026-05-18T00:26:19.141464+00:00"},{"alias_kind":"arxiv_version","alias_value":"1709.07467v2","created_at":"2026-05-18T00:26:19.141464+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1709.07467","created_at":"2026-05-18T00:26:19.141464+00:00"},{"alias_kind":"pith_short_12","alias_value":"AH5CDLSWLOEP","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_16","alias_value":"AH5CDLSWLOEPGJMQ","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_8","alias_value":"AH5CDLSW","created_at":"2026-05-18T12:31:05.417338+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.15772","citing_title":"Accretion Effects on Primordial Black Hole Reheating Constraints","ref_index":48,"is_internal_anchor":true},{"citing_arxiv_id":"2605.18097","citing_title":"Effects of formation channels and gravitational lensing on stochastic gravitational wave background","ref_index":78,"is_internal_anchor":true},{"citing_arxiv_id":"2604.01684","citing_title":"Smoluchowski Coagulation Equation and the Evolution of Primordial Black Hole Clusters","ref_index":30,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AH5CDLSWLOEPGJMQ53HEHYXPYF","json":"https://pith.science/pith/AH5CDLSWLOEPGJMQ53HEHYXPYF.json","graph_json":"https://pith.science/api/pith-number/AH5CDLSWLOEPGJMQ53HEHYXPYF/graph.json","events_json":"https://pith.science/api/pith-number/AH5CDLSWLOEPGJMQ53HEHYXPYF/events.json","paper":"https://pith.science/paper/AH5CDLSW"},"agent_actions":{"view_html":"https://pith.science/pith/AH5CDLSWLOEPGJMQ53HEHYXPYF","download_json":"https://pith.science/pith/AH5CDLSWLOEPGJMQ53HEHYXPYF.json","view_paper":"https://pith.science/paper/AH5CDLSW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1709.07467&json=true","fetch_graph":"https://pith.science/api/pith-number/AH5CDLSWLOEPGJMQ53HEHYXPYF/graph.json","fetch_events":"https://pith.science/api/pith-number/AH5CDLSWLOEPGJMQ53HEHYXPYF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AH5CDLSWLOEPGJMQ53HEHYXPYF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AH5CDLSWLOEPGJMQ53HEHYXPYF/action/storage_attestation","attest_author":"https://pith.science/pith/AH5CDLSWLOEPGJMQ53HEHYXPYF/action/author_attestation","sign_citation":"https://pith.science/pith/AH5CDLSWLOEPGJMQ53HEHYXPYF/action/citation_signature","submit_replication":"https://pith.science/pith/AH5CDLSWLOEPGJMQ53HEHYXPYF/action/replication_record"}},"created_at":"2026-05-18T00:26:19.141464+00:00","updated_at":"2026-05-18T00:26:19.141464+00:00"}