{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:6EOQLLOZ7SNPWKQUKU45LSDC2O","short_pith_number":"pith:6EOQLLOZ","schema_version":"1.0","canonical_sha256":"f11d05add9fc9afb2a145539d5c862d3b7704b62d5aeba1e3c95f5814773b474","source":{"kind":"arxiv","id":"2008.11184","version":3},"attestation_state":"computed","paper":{"title":"Multi-messenger Probes of Inflationary Fluctuations and Primordial Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","gr-qc","hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Caner Unal, Ely D. Kovetz, Subodh P. Patil","submitted_at":"2020-08-25T17:37:25Z","abstract_excerpt":"Next generation cosmic microwave background spectral distortion and pulsar timing array experiments have the potential to probe primordial fluctuations at small scales with remarkable sensitivity. We demonstrate the potential of these probes to either detect signatures of primordial black holes (PBHs) sourced from primordial overdensities within the standard thermal history of the universe over a 13-decade mass range ${\\cal O}(0.1-10^{12})M_\\odot$, or constrain their existence to a negligible abundance. Our conclusions are based only on global cosmological signals, and are robust under changes"},"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":"2008.11184","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2020-08-25T17:37:25Z","cross_cats_sorted":["astro-ph.GA","gr-qc","hep-ph","hep-th"],"title_canon_sha256":"5e7f5128f605d86e95b1a41d9dfae8b59ef0f4d5540d40ce8f10f97543b121ad","abstract_canon_sha256":"3b1d58c242212cb074c912f99a8c0cb90a8ff16935909e4056d8678d9ca01e89"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:42:27.259230Z","signature_b64":"TYJoM4NObVtzIuuuNOxK742JSrQwSaUUhsYDNi3ffr/unUtOTl+gX5rjS3V5uXxQV1myM5svqN5vpg0LiFDPCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f11d05add9fc9afb2a145539d5c862d3b7704b62d5aeba1e3c95f5814773b474","last_reissued_at":"2026-07-05T08:42:27.258698Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:42:27.258698Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multi-messenger Probes of Inflationary Fluctuations and Primordial Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","gr-qc","hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Caner Unal, Ely D. Kovetz, Subodh P. Patil","submitted_at":"2020-08-25T17:37:25Z","abstract_excerpt":"Next generation cosmic microwave background spectral distortion and pulsar timing array experiments have the potential to probe primordial fluctuations at small scales with remarkable sensitivity. We demonstrate the potential of these probes to either detect signatures of primordial black holes (PBHs) sourced from primordial overdensities within the standard thermal history of the universe over a 13-decade mass range ${\\cal O}(0.1-10^{12})M_\\odot$, or constrain their existence to a negligible abundance. Our conclusions are based only on global cosmological signals, and are robust under changes"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2008.11184","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/2008.11184/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":"2008.11184","created_at":"2026-07-05T08:42:27.258770+00:00"},{"alias_kind":"arxiv_version","alias_value":"2008.11184v3","created_at":"2026-07-05T08:42:27.258770+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2008.11184","created_at":"2026-07-05T08:42:27.258770+00:00"},{"alias_kind":"pith_short_12","alias_value":"6EOQLLOZ7SNP","created_at":"2026-07-05T08:42:27.258770+00:00"},{"alias_kind":"pith_short_16","alias_value":"6EOQLLOZ7SNPWKQU","created_at":"2026-07-05T08:42:27.258770+00:00"},{"alias_kind":"pith_short_8","alias_value":"6EOQLLOZ","created_at":"2026-07-05T08:42:27.258770+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.28296","citing_title":"Memoirs of the curvaton: non-perturbative non-Gaussianity and supermassive primordial black holes","ref_index":72,"is_internal_anchor":false},{"citing_arxiv_id":"2505.16820","citing_title":"Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order","ref_index":172,"is_internal_anchor":false},{"citing_arxiv_id":"2109.01398","citing_title":"Scalar induced gravitational waves review","ref_index":32,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6EOQLLOZ7SNPWKQUKU45LSDC2O","json":"https://pith.science/pith/6EOQLLOZ7SNPWKQUKU45LSDC2O.json","graph_json":"https://pith.science/api/pith-number/6EOQLLOZ7SNPWKQUKU45LSDC2O/graph.json","events_json":"https://pith.science/api/pith-number/6EOQLLOZ7SNPWKQUKU45LSDC2O/events.json","paper":"https://pith.science/paper/6EOQLLOZ"},"agent_actions":{"view_html":"https://pith.science/pith/6EOQLLOZ7SNPWKQUKU45LSDC2O","download_json":"https://pith.science/pith/6EOQLLOZ7SNPWKQUKU45LSDC2O.json","view_paper":"https://pith.science/paper/6EOQLLOZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2008.11184&json=true","fetch_graph":"https://pith.science/api/pith-number/6EOQLLOZ7SNPWKQUKU45LSDC2O/graph.json","fetch_events":"https://pith.science/api/pith-number/6EOQLLOZ7SNPWKQUKU45LSDC2O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6EOQLLOZ7SNPWKQUKU45LSDC2O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6EOQLLOZ7SNPWKQUKU45LSDC2O/action/storage_attestation","attest_author":"https://pith.science/pith/6EOQLLOZ7SNPWKQUKU45LSDC2O/action/author_attestation","sign_citation":"https://pith.science/pith/6EOQLLOZ7SNPWKQUKU45LSDC2O/action/citation_signature","submit_replication":"https://pith.science/pith/6EOQLLOZ7SNPWKQUKU45LSDC2O/action/replication_record"}},"created_at":"2026-07-05T08:42:27.258770+00:00","updated_at":"2026-07-05T08:42:27.258770+00:00"}