{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:NYM6IODZ5ATMOWMIR2WT72AT7C","short_pith_number":"pith:NYM6IODZ","schema_version":"1.0","canonical_sha256":"6e19e43879e826c759888ead3fe813f8b8f4b4f04ff06ac7a9ec947e77870bf8","source":{"kind":"arxiv","id":"2202.00700","version":3},"attestation_state":"computed","paper":{"title":"Induced gravitational waves from the cosmic coincidence","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Joseph Silk, Shyam Balaji, Yi-Peng Wu","submitted_at":"2022-02-01T19:00:07Z","abstract_excerpt":"The induced gravitational wave (GW) background from enhanced primordial scalar perturbations is one of the most promising observational consequences of primordial black hole (PBH) formation from inflation. We investigate the induced GW spectrum $\\Omega_{\\textrm{IGW}}$ from single-field inflation in the general ultra-slow-roll (USR) framework, restricting the peak frequency band to be inside $10^{-3}$-$1$ Hz and saturating PBH abundance to comprise all dark matter (DM) in the ultralight asteroid-mass window. By invoking successful baryogenesis driven by USR inflation, we verify the viable param"},"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":"2202.00700","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2022-02-01T19:00:07Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"860e57fa5ad1a20a42f8a1f3f87c63036a08e9a2c0c8f4d5b1cec4d0bbe99a28","abstract_canon_sha256":"72278793d67b8406aa349f0569a0cbc03f68e46115260746d540b2b5b8bb0dbf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:38:47.459016Z","signature_b64":"GNgjMSeKX3HgEl/cqLFvjEUZTMfQwIFPbhLVJnz5gR+Hr6fY2iNozhtIIwDs7OPo6FY9HwsJra1+B8aCFZriBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6e19e43879e826c759888ead3fe813f8b8f4b4f04ff06ac7a9ec947e77870bf8","last_reissued_at":"2026-07-05T04:38:47.458658Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:38:47.458658Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Induced gravitational waves from the cosmic coincidence","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Joseph Silk, Shyam Balaji, Yi-Peng Wu","submitted_at":"2022-02-01T19:00:07Z","abstract_excerpt":"The induced gravitational wave (GW) background from enhanced primordial scalar perturbations is one of the most promising observational consequences of primordial black hole (PBH) formation from inflation. We investigate the induced GW spectrum $\\Omega_{\\textrm{IGW}}$ from single-field inflation in the general ultra-slow-roll (USR) framework, restricting the peak frequency band to be inside $10^{-3}$-$1$ Hz and saturating PBH abundance to comprise all dark matter (DM) in the ultralight asteroid-mass window. By invoking successful baryogenesis driven by USR inflation, we verify the viable param"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2202.00700","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/2202.00700/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":"2202.00700","created_at":"2026-07-05T04:38:47.458721+00:00"},{"alias_kind":"arxiv_version","alias_value":"2202.00700v3","created_at":"2026-07-05T04:38:47.458721+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2202.00700","created_at":"2026-07-05T04:38:47.458721+00:00"},{"alias_kind":"pith_short_12","alias_value":"NYM6IODZ5ATM","created_at":"2026-07-05T04:38:47.458721+00:00"},{"alias_kind":"pith_short_16","alias_value":"NYM6IODZ5ATMOWMI","created_at":"2026-07-05T04:38:47.458721+00:00"},{"alias_kind":"pith_short_8","alias_value":"NYM6IODZ","created_at":"2026-07-05T04:38:47.458721+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.14044","citing_title":"The Magnetic Origin of Primordial Black Holes: Ultralight PBHs and Secondary GWs","ref_index":90,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NYM6IODZ5ATMOWMIR2WT72AT7C","json":"https://pith.science/pith/NYM6IODZ5ATMOWMIR2WT72AT7C.json","graph_json":"https://pith.science/api/pith-number/NYM6IODZ5ATMOWMIR2WT72AT7C/graph.json","events_json":"https://pith.science/api/pith-number/NYM6IODZ5ATMOWMIR2WT72AT7C/events.json","paper":"https://pith.science/paper/NYM6IODZ"},"agent_actions":{"view_html":"https://pith.science/pith/NYM6IODZ5ATMOWMIR2WT72AT7C","download_json":"https://pith.science/pith/NYM6IODZ5ATMOWMIR2WT72AT7C.json","view_paper":"https://pith.science/paper/NYM6IODZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2202.00700&json=true","fetch_graph":"https://pith.science/api/pith-number/NYM6IODZ5ATMOWMIR2WT72AT7C/graph.json","fetch_events":"https://pith.science/api/pith-number/NYM6IODZ5ATMOWMIR2WT72AT7C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NYM6IODZ5ATMOWMIR2WT72AT7C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NYM6IODZ5ATMOWMIR2WT72AT7C/action/storage_attestation","attest_author":"https://pith.science/pith/NYM6IODZ5ATMOWMIR2WT72AT7C/action/author_attestation","sign_citation":"https://pith.science/pith/NYM6IODZ5ATMOWMIR2WT72AT7C/action/citation_signature","submit_replication":"https://pith.science/pith/NYM6IODZ5ATMOWMIR2WT72AT7C/action/replication_record"}},"created_at":"2026-07-05T04:38:47.458721+00:00","updated_at":"2026-07-05T04:38:47.458721+00:00"}