{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:LRDCXGORQIPQPSCWYMMDVCQPHZ","short_pith_number":"pith:LRDCXGOR","schema_version":"1.0","canonical_sha256":"5c462b99d1821f07c856c3183a8a0f3e471eab87a9f438c499c74b3e6699c2b3","source":{"kind":"arxiv","id":"2307.11639","version":2},"attestation_state":"computed","paper":{"title":"Primordial black holes as dark matter: Interferometric tests of phase transition origin","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Iason Baldes, Mar\\'ia Olalla Olea-Romacho","submitted_at":"2023-07-21T15:10:41Z","abstract_excerpt":"We show that primordial black holes - in the observationally allowed mass window with $f_{\\rm pbh}=1$ - formed from late nucleating patches in a first order phase transition imply upcoming gravitational wave interferometers will see a large stochastic background arising from the bubble collisions. As an example, we use a classically scale invariant $B-L$ model, in which the right handed neutrinos explain the neutrino masses and leptogenesis, and the dark matter consists of primordial black holes. The conclusion regarding the gravitational waves is, however, expected to hold model independently"},"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":"2307.11639","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2023-07-21T15:10:41Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"8bcd22bc12275d9600415f2380cfdfb80ac86677d57aadbcb3afba30259cbd7d","abstract_canon_sha256":"bc6961ca08d77940fd1ccd805c4a55124f2560d8a880fe91564e457a5ef38f8e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:37:12.220926Z","signature_b64":"cuYBh35tSQzetIgV2yBMFh06eNnCjISHmJltnn6u0Bi0JRjTOE3kC8w4jD+ne8C53yW0hNmlx62xjwSZ1rABAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5c462b99d1821f07c856c3183a8a0f3e471eab87a9f438c499c74b3e6699c2b3","last_reissued_at":"2026-07-05T07:37:12.220431Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:37:12.220431Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Primordial black holes as dark matter: Interferometric tests of phase transition origin","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Iason Baldes, Mar\\'ia Olalla Olea-Romacho","submitted_at":"2023-07-21T15:10:41Z","abstract_excerpt":"We show that primordial black holes - in the observationally allowed mass window with $f_{\\rm pbh}=1$ - formed from late nucleating patches in a first order phase transition imply upcoming gravitational wave interferometers will see a large stochastic background arising from the bubble collisions. As an example, we use a classically scale invariant $B-L$ model, in which the right handed neutrinos explain the neutrino masses and leptogenesis, and the dark matter consists of primordial black holes. The conclusion regarding the gravitational waves is, however, expected to hold model independently"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2307.11639","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/2307.11639/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":"2307.11639","created_at":"2026-07-05T07:37:12.220490+00:00"},{"alias_kind":"arxiv_version","alias_value":"2307.11639v2","created_at":"2026-07-05T07:37:12.220490+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2307.11639","created_at":"2026-07-05T07:37:12.220490+00:00"},{"alias_kind":"pith_short_12","alias_value":"LRDCXGORQIPQ","created_at":"2026-07-05T07:37:12.220490+00:00"},{"alias_kind":"pith_short_16","alias_value":"LRDCXGORQIPQPSCW","created_at":"2026-07-05T07:37:12.220490+00:00"},{"alias_kind":"pith_short_8","alias_value":"LRDCXGOR","created_at":"2026-07-05T07:37:12.220490+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":11,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.09482","citing_title":"Primordial Black Holes from Slow Phase Transitions with Delayed Reheating: A Peak-Theory Approach","ref_index":16,"is_internal_anchor":false},{"citing_arxiv_id":"2606.07505","citing_title":"Primordial Black Hole Triggered Type Ia Supernovae II: Comparison with Supernova Remnants and Galactic Chemical Evolution","ref_index":190,"is_internal_anchor":false},{"citing_arxiv_id":"2606.01580","citing_title":"Primordial black holes spin from cosmological first-order phase transitions","ref_index":45,"is_internal_anchor":false},{"citing_arxiv_id":"2606.01580","citing_title":"Primordial black holes spin from cosmological first-order phase transitions","ref_index":39,"is_internal_anchor":false},{"citing_arxiv_id":"2506.15496","citing_title":"Thermodynamical uncertainties for primordial black holes from cosmological phase transitions","ref_index":62,"is_internal_anchor":false},{"citing_arxiv_id":"2503.01962","citing_title":"Curvature Perturbations from First-Order Phase Transitions: Implications to Black Holes and Gravitational Waves","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"2505.08011","citing_title":"Primordial black holes and magnetic fields in conformal neutrino mass models","ref_index":9,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11332","citing_title":"Reviving primordial black hole formation in slow first-order phase transitions","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2603.09126","citing_title":"Dark matter in classically conformal theories: WIMP and supercooling","ref_index":58,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21474","citing_title":"Gravitational Waves from Black Hole Reheating: The Scalar-Induced Component","ref_index":80,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11332","citing_title":"Reviving primordial black hole formation in slow first-order phase transitions","ref_index":18,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LRDCXGORQIPQPSCWYMMDVCQPHZ","json":"https://pith.science/pith/LRDCXGORQIPQPSCWYMMDVCQPHZ.json","graph_json":"https://pith.science/api/pith-number/LRDCXGORQIPQPSCWYMMDVCQPHZ/graph.json","events_json":"https://pith.science/api/pith-number/LRDCXGORQIPQPSCWYMMDVCQPHZ/events.json","paper":"https://pith.science/paper/LRDCXGOR"},"agent_actions":{"view_html":"https://pith.science/pith/LRDCXGORQIPQPSCWYMMDVCQPHZ","download_json":"https://pith.science/pith/LRDCXGORQIPQPSCWYMMDVCQPHZ.json","view_paper":"https://pith.science/paper/LRDCXGOR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2307.11639&json=true","fetch_graph":"https://pith.science/api/pith-number/LRDCXGORQIPQPSCWYMMDVCQPHZ/graph.json","fetch_events":"https://pith.science/api/pith-number/LRDCXGORQIPQPSCWYMMDVCQPHZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LRDCXGORQIPQPSCWYMMDVCQPHZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LRDCXGORQIPQPSCWYMMDVCQPHZ/action/storage_attestation","attest_author":"https://pith.science/pith/LRDCXGORQIPQPSCWYMMDVCQPHZ/action/author_attestation","sign_citation":"https://pith.science/pith/LRDCXGORQIPQPSCWYMMDVCQPHZ/action/citation_signature","submit_replication":"https://pith.science/pith/LRDCXGORQIPQPSCWYMMDVCQPHZ/action/replication_record"}},"created_at":"2026-07-05T07:37:12.220490+00:00","updated_at":"2026-07-05T07:37:12.220490+00:00"}