{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:ENM7KORNI2VBCHJGCNBRATAX33","short_pith_number":"pith:ENM7KORN","schema_version":"1.0","canonical_sha256":"2359f53a2d46aa111d261343104c17def4c014e117932a23c24f8e37288221cc","source":{"kind":"arxiv","id":"2607.27338","version":1},"attestation_state":"computed","paper":{"title":"Gravitational Waves as a Source of Large-Scale White Noise: New Constraints","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Albert Stebbins, Gabriela Barenboim","submitted_at":"2026-07-29T18:00:27Z","abstract_excerpt":"A stochastic gravitational wave (GW) background sources a shear in the flow of cosmic fluid which, through non-linear mode coupling, generates large-scale white noise (LSWN) in the kurvature density field. Building on the LSWN framework of our previous work, we derive the amplitude of this GW-induced LSWN and translate the observational non-detection of LSWN into bounds on the production redshift and density of gravity waves. In particular, a minimal constraint on gravity waves with $z=0$ density parameter $\\Omega_\\mathrm{GW0}^*$ in frequency band $f_*$ generated at redshift $z_*$ must satisfy"},"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":"2607.27338","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-07-29T18:00:27Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"3e34b48a6f4808dddac58fa17cf7a1a4598aaf843b229d1d2d490253e0874e84","abstract_canon_sha256":"4385f4fc20946e24f3cee4233b825e47b0c61f538dc5ad6ee01f524a35b3b3b7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2359f53a2d46aa111d261343104c17def4c014e117932a23c24f8e37288221cc","last_reissued_at":"2026-07-31T00:10:42.072041Z","signature_status":"unsigned_v0","first_computed_at":"2026-07-31T00:10:42.072041Z"},"graph_snapshot":{"paper":{"title":"Gravitational Waves as a Source of Large-Scale White Noise: New Constraints","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Albert Stebbins, Gabriela Barenboim","submitted_at":"2026-07-29T18:00:27Z","abstract_excerpt":"A stochastic gravitational wave (GW) background sources a shear in the flow of cosmic fluid which, through non-linear mode coupling, generates large-scale white noise (LSWN) in the kurvature density field. Building on the LSWN framework of our previous work, we derive the amplitude of this GW-induced LSWN and translate the observational non-detection of LSWN into bounds on the production redshift and density of gravity waves. In particular, a minimal constraint on gravity waves with $z=0$ density parameter $\\Omega_\\mathrm{GW0}^*$ in frequency band $f_*$ generated at redshift $z_*$ must satisfy"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2607.27338","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/2607.27338/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":"2607.27338","created_at":"2026-07-31T00:10:42.074344+00:00"},{"alias_kind":"arxiv_version","alias_value":"2607.27338v1","created_at":"2026-07-31T00:10:42.074344+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2607.27338","created_at":"2026-07-31T00:10:42.074344+00:00"},{"alias_kind":"pith_short_12","alias_value":"ENM7KORNI2VB","created_at":"2026-07-31T00:10:42.074344+00:00"},{"alias_kind":"pith_short_16","alias_value":"ENM7KORNI2VBCHJG","created_at":"2026-07-31T00:10:42.074344+00:00"},{"alias_kind":"pith_short_8","alias_value":"ENM7KORN","created_at":"2026-07-31T00:10:42.074344+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ENM7KORNI2VBCHJGCNBRATAX33","json":"https://pith.science/pith/ENM7KORNI2VBCHJGCNBRATAX33.json","graph_json":"https://pith.science/api/pith-number/ENM7KORNI2VBCHJGCNBRATAX33/graph.json","events_json":"https://pith.science/api/pith-number/ENM7KORNI2VBCHJGCNBRATAX33/events.json","paper":"https://pith.science/paper/ENM7KORN"},"agent_actions":{"view_html":"https://pith.science/pith/ENM7KORNI2VBCHJGCNBRATAX33","download_json":"https://pith.science/pith/ENM7KORNI2VBCHJGCNBRATAX33.json","view_paper":"https://pith.science/paper/ENM7KORN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2607.27338&json=true","fetch_graph":"https://pith.science/api/pith-number/ENM7KORNI2VBCHJGCNBRATAX33/graph.json","fetch_events":"https://pith.science/api/pith-number/ENM7KORNI2VBCHJGCNBRATAX33/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ENM7KORNI2VBCHJGCNBRATAX33/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ENM7KORNI2VBCHJGCNBRATAX33/action/storage_attestation","attest_author":"https://pith.science/pith/ENM7KORNI2VBCHJGCNBRATAX33/action/author_attestation","sign_citation":"https://pith.science/pith/ENM7KORNI2VBCHJGCNBRATAX33/action/citation_signature","submit_replication":"https://pith.science/pith/ENM7KORNI2VBCHJGCNBRATAX33/action/replication_record"}},"created_at":"2026-07-31T00:10:42.074344+00:00","updated_at":"2026-07-31T00:10:42.074344+00:00"}