{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:LG67T3N5SMCHBYVUEUHNNPITPJ","short_pith_number":"pith:LG67T3N5","schema_version":"1.0","canonical_sha256":"59bdf9edbd930470e2b4250ed6bd137a5e204856c479c43ea5ff892df79c0a54","source":{"kind":"arxiv","id":"2302.10188","version":1},"attestation_state":"computed","paper":{"title":"Primordial Gravitational Waves From Black Hole Evaporation in Standard and Non-Standard Cosmologies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE","hep-ph"],"primary_cat":"gr-qc","authors_text":"Aurora Ireland, Jordan Scharnhorst, Stefano Profumo","submitted_at":"2023-02-17T19:00:08Z","abstract_excerpt":"Gravitons radiated from light, evaporating black holes contribute to the stochastic background of gravitational waves. The spectrum of such emission depends on both the mass and the spin of the black holes, as well as on the redshifting that occurs between the black hole formation and today. This, in turn, depends on the expansion history of the universe, which is largely unknown and unconstrained at times prior to the synthesis of light elements. Here, we explore the features of the stochastic background of gravitational waves from black hole evaporation under a broad range of possible early "},"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":"2302.10188","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2023-02-17T19:00:08Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE","hep-ph"],"title_canon_sha256":"6f2450b53e2c48fdd21c29b9a3254545ef9df4741f163d82bb57a77e962c29f4","abstract_canon_sha256":"41fe7ba6b45200826edc8909d578121f29109deb48cae1c8a56eb13f87751c3a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:08:21.231664Z","signature_b64":"8ERxn85NVvebbXs+z9NPVjUIrnqVaXbg1dIl0CPAXUvbLlwuev6HLi+Kr+Hn7ZA9KlO808MoyAoClvIJw4qaBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"59bdf9edbd930470e2b4250ed6bd137a5e204856c479c43ea5ff892df79c0a54","last_reissued_at":"2026-07-05T06:08:21.231182Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:08:21.231182Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Primordial Gravitational Waves From Black Hole Evaporation in Standard and Non-Standard Cosmologies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE","hep-ph"],"primary_cat":"gr-qc","authors_text":"Aurora Ireland, Jordan Scharnhorst, Stefano Profumo","submitted_at":"2023-02-17T19:00:08Z","abstract_excerpt":"Gravitons radiated from light, evaporating black holes contribute to the stochastic background of gravitational waves. The spectrum of such emission depends on both the mass and the spin of the black holes, as well as on the redshifting that occurs between the black hole formation and today. This, in turn, depends on the expansion history of the universe, which is largely unknown and unconstrained at times prior to the synthesis of light elements. Here, we explore the features of the stochastic background of gravitational waves from black hole evaporation under a broad range of possible early "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2302.10188","kind":"arxiv","version":1},"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/2302.10188/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":"2302.10188","created_at":"2026-07-05T06:08:21.231238+00:00"},{"alias_kind":"arxiv_version","alias_value":"2302.10188v1","created_at":"2026-07-05T06:08:21.231238+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2302.10188","created_at":"2026-07-05T06:08:21.231238+00:00"},{"alias_kind":"pith_short_12","alias_value":"LG67T3N5SMCH","created_at":"2026-07-05T06:08:21.231238+00:00"},{"alias_kind":"pith_short_16","alias_value":"LG67T3N5SMCHBYVU","created_at":"2026-07-05T06:08:21.231238+00:00"},{"alias_kind":"pith_short_8","alias_value":"LG67T3N5","created_at":"2026-07-05T06:08:21.231238+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.19825","citing_title":"Inflaton Accretion onto Primordial Black Holes During Reheating","ref_index":102,"is_internal_anchor":false},{"citing_arxiv_id":"2511.01848","citing_title":"Constraining memory-burdened primordial black holes with graviton-photon conversion and binary mergers","ref_index":19,"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":170,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LG67T3N5SMCHBYVUEUHNNPITPJ","json":"https://pith.science/pith/LG67T3N5SMCHBYVUEUHNNPITPJ.json","graph_json":"https://pith.science/api/pith-number/LG67T3N5SMCHBYVUEUHNNPITPJ/graph.json","events_json":"https://pith.science/api/pith-number/LG67T3N5SMCHBYVUEUHNNPITPJ/events.json","paper":"https://pith.science/paper/LG67T3N5"},"agent_actions":{"view_html":"https://pith.science/pith/LG67T3N5SMCHBYVUEUHNNPITPJ","download_json":"https://pith.science/pith/LG67T3N5SMCHBYVUEUHNNPITPJ.json","view_paper":"https://pith.science/paper/LG67T3N5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2302.10188&json=true","fetch_graph":"https://pith.science/api/pith-number/LG67T3N5SMCHBYVUEUHNNPITPJ/graph.json","fetch_events":"https://pith.science/api/pith-number/LG67T3N5SMCHBYVUEUHNNPITPJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LG67T3N5SMCHBYVUEUHNNPITPJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LG67T3N5SMCHBYVUEUHNNPITPJ/action/storage_attestation","attest_author":"https://pith.science/pith/LG67T3N5SMCHBYVUEUHNNPITPJ/action/author_attestation","sign_citation":"https://pith.science/pith/LG67T3N5SMCHBYVUEUHNNPITPJ/action/citation_signature","submit_replication":"https://pith.science/pith/LG67T3N5SMCHBYVUEUHNNPITPJ/action/replication_record"}},"created_at":"2026-07-05T06:08:21.231238+00:00","updated_at":"2026-07-05T06:08:21.231238+00:00"}