{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:HUXUOJWFXJXAWJCO5LCYW6NTMN","short_pith_number":"pith:HUXUOJWF","schema_version":"1.0","canonical_sha256":"3d2f4726c5ba6e0b244eeac58b79b3636c2ed5f9daafa43b3f4a7e365b08b7fe","source":{"kind":"arxiv","id":"2105.06816","version":2},"attestation_state":"computed","paper":{"title":"Exploring Evaporating Primordial Black Holes with Gravitational Waves","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Guillem Dom\\`enech, Misao Sasaki, Volodymyr Takhistov","submitted_at":"2021-05-14T13:23:58Z","abstract_excerpt":"Primordial black holes (PBHs) from the early Universe have been connected with the nature of dark matter and can significantly affect cosmological history. We show that coincidence dark radiation and density fluctuation gravitational wave signatures associated with evaporation of $\\lesssim10^9$ g PBHs can be used to explore and obtain important hints about the formation mechanisms of spinning and non-spinning PBHs spanning orders of magnitude in mass-range, which is challenging to do otherwise."},"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":"2105.06816","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2021-05-14T13:23:58Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"6addec7c9f8a6afbf31a7422c0acad0d20eca405c585ff36261007d3814b6949","abstract_canon_sha256":"4bba5822b9d5e11e60cefd710222523b8bb8e3a693c67fd8f36c24f1cd7a22a5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:29:16.331536Z","signature_b64":"HWwhXimjM218ytnrXSWFiZKY/NqTfqt5+PlLN+rW6OHEazKQIUouVYSWbxDjGWKJL1Rfq1ZSD7Nha4F/826sBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3d2f4726c5ba6e0b244eeac58b79b3636c2ed5f9daafa43b3f4a7e365b08b7fe","last_reissued_at":"2026-07-05T03:29:16.331074Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:29:16.331074Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Exploring Evaporating Primordial Black Holes with Gravitational Waves","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Guillem Dom\\`enech, Misao Sasaki, Volodymyr Takhistov","submitted_at":"2021-05-14T13:23:58Z","abstract_excerpt":"Primordial black holes (PBHs) from the early Universe have been connected with the nature of dark matter and can significantly affect cosmological history. We show that coincidence dark radiation and density fluctuation gravitational wave signatures associated with evaporation of $\\lesssim10^9$ g PBHs can be used to explore and obtain important hints about the formation mechanisms of spinning and non-spinning PBHs spanning orders of magnitude in mass-range, which is challenging to do otherwise."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2105.06816","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/2105.06816/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":"2105.06816","created_at":"2026-07-05T03:29:16.331132+00:00"},{"alias_kind":"arxiv_version","alias_value":"2105.06816v2","created_at":"2026-07-05T03:29:16.331132+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2105.06816","created_at":"2026-07-05T03:29:16.331132+00:00"},{"alias_kind":"pith_short_12","alias_value":"HUXUOJWFXJXA","created_at":"2026-07-05T03:29:16.331132+00:00"},{"alias_kind":"pith_short_16","alias_value":"HUXUOJWFXJXAWJCO","created_at":"2026-07-05T03:29:16.331132+00:00"},{"alias_kind":"pith_short_8","alias_value":"HUXUOJWF","created_at":"2026-07-05T03:29:16.331132+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.23787","citing_title":"Multi-peaked high-frequency gravitational waves from PBH-assisted leptogenesis","ref_index":80,"is_internal_anchor":false},{"citing_arxiv_id":"2606.09804","citing_title":"Universal Suppression of Gravitational Waves from Black Hole Evaporation Dynamics","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21474","citing_title":"Gravitational Waves from Black Hole Reheating: The Scalar-Induced Component","ref_index":211,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21477","citing_title":"Opening the Window of Ultra-Light PBHs by Exorcising the Poltergeist","ref_index":31,"is_internal_anchor":false},{"citing_arxiv_id":"2109.01398","citing_title":"Scalar induced gravitational waves review","ref_index":71,"is_internal_anchor":false},{"citing_arxiv_id":"2605.14044","citing_title":"The Magnetic Origin of Primordial Black Holes: Ultralight PBHs and Secondary GWs","ref_index":171,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08336","citing_title":"Primordial Black Hole Hotspots Beyond Flat Spacetime","ref_index":48,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HUXUOJWFXJXAWJCO5LCYW6NTMN","json":"https://pith.science/pith/HUXUOJWFXJXAWJCO5LCYW6NTMN.json","graph_json":"https://pith.science/api/pith-number/HUXUOJWFXJXAWJCO5LCYW6NTMN/graph.json","events_json":"https://pith.science/api/pith-number/HUXUOJWFXJXAWJCO5LCYW6NTMN/events.json","paper":"https://pith.science/paper/HUXUOJWF"},"agent_actions":{"view_html":"https://pith.science/pith/HUXUOJWFXJXAWJCO5LCYW6NTMN","download_json":"https://pith.science/pith/HUXUOJWFXJXAWJCO5LCYW6NTMN.json","view_paper":"https://pith.science/paper/HUXUOJWF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2105.06816&json=true","fetch_graph":"https://pith.science/api/pith-number/HUXUOJWFXJXAWJCO5LCYW6NTMN/graph.json","fetch_events":"https://pith.science/api/pith-number/HUXUOJWFXJXAWJCO5LCYW6NTMN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HUXUOJWFXJXAWJCO5LCYW6NTMN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HUXUOJWFXJXAWJCO5LCYW6NTMN/action/storage_attestation","attest_author":"https://pith.science/pith/HUXUOJWFXJXAWJCO5LCYW6NTMN/action/author_attestation","sign_citation":"https://pith.science/pith/HUXUOJWFXJXAWJCO5LCYW6NTMN/action/citation_signature","submit_replication":"https://pith.science/pith/HUXUOJWFXJXAWJCO5LCYW6NTMN/action/replication_record"}},"created_at":"2026-07-05T03:29:16.331132+00:00","updated_at":"2026-07-05T03:29:16.331132+00:00"}