{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:U66TMIR625BBID4OZAACXDV4EA","short_pith_number":"pith:U66TMIR6","schema_version":"1.0","canonical_sha256":"a7bd36223ed742140f8ec8002b8ebc20224db4e612aff6e5226ef40633da17e3","source":{"kind":"arxiv","id":"2311.17829","version":3},"attestation_state":"computed","paper":{"title":"Coexistence Test of Primordial Black Holes and Particle Dark Matter from Diffractive Lensing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Han Gil Choi, Philip Lu, Sunghoon Jung, Volodymyr Takhistov","submitted_at":"2023-11-29T17:31:15Z","abstract_excerpt":"If dark matter (DM) consists of primordial black holes (PBHs) and particles simultaneously, PBHs are generically embedded within particle DM halos. Such ``dressed PBHs'' (dPBHs) are subject to modified constraints compared to PBHs and can contribute to significant DM abundance in the mass range $10^{-1} - 10^2 M_\\odot$. We show that diffractive lensing of chirping gravitational waves (GWs) from binary mergers can not only discover, but can also identify dPBH lenses and discriminate them from bare PBHs on the event-by-event basis, with potential to definitively establish the coexistence of subd"},"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":"2311.17829","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2023-11-29T17:31:15Z","cross_cats_sorted":["astro-ph.HE","gr-qc","hep-ph"],"title_canon_sha256":"9e1bbcd00932f0e00e895921d49ba805bcbdae6d39bcf00dd89ad963631e3b8f","abstract_canon_sha256":"216047f6d1e46db035262f35399540845250b222d9b9381ad6a7b53b9087fca1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:04:30.608473Z","signature_b64":"FdZKzzyUpdTHpwpj4h9tr+ou1l6fG4MxHp99f9s1cSkejy/Ne0FOynDb2WZcPizSkX0TSFxeUe1IgSwRL9gzBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a7bd36223ed742140f8ec8002b8ebc20224db4e612aff6e5226ef40633da17e3","last_reissued_at":"2026-07-05T09:04:30.608048Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:04:30.608048Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Coexistence Test of Primordial Black Holes and Particle Dark Matter from Diffractive Lensing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Han Gil Choi, Philip Lu, Sunghoon Jung, Volodymyr Takhistov","submitted_at":"2023-11-29T17:31:15Z","abstract_excerpt":"If dark matter (DM) consists of primordial black holes (PBHs) and particles simultaneously, PBHs are generically embedded within particle DM halos. Such ``dressed PBHs'' (dPBHs) are subject to modified constraints compared to PBHs and can contribute to significant DM abundance in the mass range $10^{-1} - 10^2 M_\\odot$. We show that diffractive lensing of chirping gravitational waves (GWs) from binary mergers can not only discover, but can also identify dPBH lenses and discriminate them from bare PBHs on the event-by-event basis, with potential to definitively establish the coexistence of subd"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.17829","kind":"arxiv","version":3},"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/2311.17829/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":"2311.17829","created_at":"2026-07-05T09:04:30.608095+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.17829v3","created_at":"2026-07-05T09:04:30.608095+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.17829","created_at":"2026-07-05T09:04:30.608095+00:00"},{"alias_kind":"pith_short_12","alias_value":"U66TMIR625BB","created_at":"2026-07-05T09:04:30.608095+00:00"},{"alias_kind":"pith_short_16","alias_value":"U66TMIR625BBID4O","created_at":"2026-07-05T09:04:30.608095+00:00"},{"alias_kind":"pith_short_8","alias_value":"U66TMIR6","created_at":"2026-07-05T09:04:30.608095+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.17765","citing_title":"Effective description of lensed gravitational waves diffracted by stellar fields","ref_index":95,"is_internal_anchor":false},{"citing_arxiv_id":"2510.27424","citing_title":"Extracting Properties of Dark Dense Environments around Black Holes from Gravitational Waves","ref_index":54,"is_internal_anchor":false},{"citing_arxiv_id":"2602.04858","citing_title":"Primordial black holes as cosmic accelerators of light dark matter: Novel direct detection constraints","ref_index":16,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/U66TMIR625BBID4OZAACXDV4EA","json":"https://pith.science/pith/U66TMIR625BBID4OZAACXDV4EA.json","graph_json":"https://pith.science/api/pith-number/U66TMIR625BBID4OZAACXDV4EA/graph.json","events_json":"https://pith.science/api/pith-number/U66TMIR625BBID4OZAACXDV4EA/events.json","paper":"https://pith.science/paper/U66TMIR6"},"agent_actions":{"view_html":"https://pith.science/pith/U66TMIR625BBID4OZAACXDV4EA","download_json":"https://pith.science/pith/U66TMIR625BBID4OZAACXDV4EA.json","view_paper":"https://pith.science/paper/U66TMIR6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.17829&json=true","fetch_graph":"https://pith.science/api/pith-number/U66TMIR625BBID4OZAACXDV4EA/graph.json","fetch_events":"https://pith.science/api/pith-number/U66TMIR625BBID4OZAACXDV4EA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/U66TMIR625BBID4OZAACXDV4EA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/U66TMIR625BBID4OZAACXDV4EA/action/storage_attestation","attest_author":"https://pith.science/pith/U66TMIR625BBID4OZAACXDV4EA/action/author_attestation","sign_citation":"https://pith.science/pith/U66TMIR625BBID4OZAACXDV4EA/action/citation_signature","submit_replication":"https://pith.science/pith/U66TMIR625BBID4OZAACXDV4EA/action/replication_record"}},"created_at":"2026-07-05T09:04:30.608095+00:00","updated_at":"2026-07-05T09:04:30.608095+00:00"}