{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:XNPBLCDHE3S4HOEQ4N5QMYY7RC","short_pith_number":"pith:XNPBLCDH","schema_version":"1.0","canonical_sha256":"bb5e15886726e5c3b890e37b06631f88b956ecf44cb5c4fff24baac54ff8ce0f","source":{"kind":"arxiv","id":"1603.05234","version":2},"attestation_state":"computed","paper":{"title":"The clustering of massive Primordial Black Holes as Dark Matter: measuring their mass distribution with Advanced LIGO","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Juan Garc\\'ia-Bellido, Sebastien Clesse","submitted_at":"2016-03-16T19:38:33Z","abstract_excerpt":"The recent detection by Advanced LIGO of gravitational waves (GW) from the merging of a binary black hole system sets new limits on the merging rates of massive primordial black holes (PBH) that could be a significant fraction or even the totality of the dark matter in the Universe. aLIGO opens the way to the determination of the distribution and clustering of such massive PBH. If PBH clusters have a similar density to the one observed in ultra-faint dwarf galaxies, we find merging rates comparable to aLIGO expectations. Massive PBH dark matter predicts the existence of thousands of those dwar"},"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":"1603.05234","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-03-16T19:38:33Z","cross_cats_sorted":["astro-ph.GA","hep-th"],"title_canon_sha256":"5cabde3e776f9f78ea0cc314b497256c29220d74a4eaf8b88ebd3a1813c39727","abstract_canon_sha256":"7d89ee857bfb806aed1d9f9dd89d44b2fb19898cb9208863a119d843f50ca78a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:00:39.540602Z","signature_b64":"YJjDYCc38YJVol1UBGErfuz/2aXFGxP5YY0jWyLdZ7USkWtL6KzNCs48mc/TVchXYDfh+uEIV6iGCX4FUjQMAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bb5e15886726e5c3b890e37b06631f88b956ecf44cb5c4fff24baac54ff8ce0f","last_reissued_at":"2026-05-18T01:00:39.540039Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:00:39.540039Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The clustering of massive Primordial Black Holes as Dark Matter: measuring their mass distribution with Advanced LIGO","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Juan Garc\\'ia-Bellido, Sebastien Clesse","submitted_at":"2016-03-16T19:38:33Z","abstract_excerpt":"The recent detection by Advanced LIGO of gravitational waves (GW) from the merging of a binary black hole system sets new limits on the merging rates of massive primordial black holes (PBH) that could be a significant fraction or even the totality of the dark matter in the Universe. aLIGO opens the way to the determination of the distribution and clustering of such massive PBH. If PBH clusters have a similar density to the one observed in ultra-faint dwarf galaxies, we find merging rates comparable to aLIGO expectations. Massive PBH dark matter predicts the existence of thousands of those dwar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.05234","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":"1603.05234","created_at":"2026-05-18T01:00:39.540126+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.05234v2","created_at":"2026-05-18T01:00:39.540126+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.05234","created_at":"2026-05-18T01:00:39.540126+00:00"},{"alias_kind":"pith_short_12","alias_value":"XNPBLCDHE3S4","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_16","alias_value":"XNPBLCDHE3S4HOEQ","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_8","alias_value":"XNPBLCDH","created_at":"2026-05-18T12:30:51.357362+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":13,"internal_anchor_count":9,"sample":[{"citing_arxiv_id":"2502.20166","citing_title":"Numerical simulations of density perturbation and gravitational wave production from cosmological first-order phase transition","ref_index":29,"is_internal_anchor":true},{"citing_arxiv_id":"2605.22789","citing_title":"Primordial black holes in excursion set theory: Formation probabilities, mass functions, and window functions","ref_index":8,"is_internal_anchor":true},{"citing_arxiv_id":"2605.19825","citing_title":"Inflaton Accretion onto Primordial Black Holes During Reheating","ref_index":15,"is_internal_anchor":true},{"citing_arxiv_id":"2508.09965","citing_title":"GW231123: A Possible Primordial Black Hole Origin","ref_index":33,"is_internal_anchor":true},{"citing_arxiv_id":"2303.15923","citing_title":"Science with the Einstein Telescope: a comparison of different designs","ref_index":265,"is_internal_anchor":true},{"citing_arxiv_id":"1912.02622","citing_title":"Science Case for the Einstein Telescope","ref_index":33,"is_internal_anchor":true},{"citing_arxiv_id":"2602.15974","citing_title":"Stellar microlensing surveys as a probe of Primordial Black Holes: status and prospects","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2605.15197","citing_title":"Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls","ref_index":76,"is_internal_anchor":true},{"citing_arxiv_id":"2002.12778","citing_title":"Constraints on Primordial Black Holes","ref_index":283,"is_internal_anchor":true},{"citing_arxiv_id":"2604.22731","citing_title":"Precision Analysis for $\\boldsymbol{H_0}$ Using Upcoming Multi-band Gravitational Wave Observations","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"2604.22462","citing_title":"Machine Learning for Multi-messenger Probes of New Physics and Cosmology: A Review and Perspective","ref_index":155,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06858","citing_title":"Memory-Burden Suppression of Hawking Radiation and Neutrino Constraints on Primordial Black Holes","ref_index":26,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14871","citing_title":"Microscopic primordial black holes as macroscopic dark matter from large extra dimensions","ref_index":53,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XNPBLCDHE3S4HOEQ4N5QMYY7RC","json":"https://pith.science/pith/XNPBLCDHE3S4HOEQ4N5QMYY7RC.json","graph_json":"https://pith.science/api/pith-number/XNPBLCDHE3S4HOEQ4N5QMYY7RC/graph.json","events_json":"https://pith.science/api/pith-number/XNPBLCDHE3S4HOEQ4N5QMYY7RC/events.json","paper":"https://pith.science/paper/XNPBLCDH"},"agent_actions":{"view_html":"https://pith.science/pith/XNPBLCDHE3S4HOEQ4N5QMYY7RC","download_json":"https://pith.science/pith/XNPBLCDHE3S4HOEQ4N5QMYY7RC.json","view_paper":"https://pith.science/paper/XNPBLCDH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.05234&json=true","fetch_graph":"https://pith.science/api/pith-number/XNPBLCDHE3S4HOEQ4N5QMYY7RC/graph.json","fetch_events":"https://pith.science/api/pith-number/XNPBLCDHE3S4HOEQ4N5QMYY7RC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XNPBLCDHE3S4HOEQ4N5QMYY7RC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XNPBLCDHE3S4HOEQ4N5QMYY7RC/action/storage_attestation","attest_author":"https://pith.science/pith/XNPBLCDHE3S4HOEQ4N5QMYY7RC/action/author_attestation","sign_citation":"https://pith.science/pith/XNPBLCDHE3S4HOEQ4N5QMYY7RC/action/citation_signature","submit_replication":"https://pith.science/pith/XNPBLCDHE3S4HOEQ4N5QMYY7RC/action/replication_record"}},"created_at":"2026-05-18T01:00:39.540126+00:00","updated_at":"2026-05-18T01:00:39.540126+00:00"}