{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:RROX3EYMWLNTYCK7WPL54AIKXH","short_pith_number":"pith:RROX3EYM","schema_version":"1.0","canonical_sha256":"8c5d7d930cb2db3c095fb3d7de010ab9d7bbfdc79cce6407973e5ca049c7df92","source":{"kind":"arxiv","id":"2310.19448","version":3},"attestation_state":"computed","paper":{"title":"The Astrophysical Gravitational Wave Background in the mHz band is likely dominated by White Dwarf binaries","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Gijs Nelemans, Seppe Staelens","submitted_at":"2023-10-30T11:17:56Z","abstract_excerpt":"Context. The Astrophysical Gravitational Wave Background (AGWB) is a collective signal of astrophysical gravitational wave sources and is dominated by compact binaries. Its measurement is one of the science goals of current and future gravitational wave detectors. Aims. We aim to determine what population of compact binaries dominates the AGWB in the mHz band. Methods. We revisit and update earlier work by Farmer & Phinney (2003) to model the astrophysical gravitational wave background sourced by extragalactic white dwarf binaries in the mHz frequency band. We calculate the signal using a sing"},"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":"2310.19448","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-10-30T11:17:56Z","cross_cats_sorted":["astro-ph.CO","gr-qc"],"title_canon_sha256":"12339369ed2827aca72c8b4091e8500a7fcc0ab986a89cf0fdaa2b3e35b3193d","abstract_canon_sha256":"226667933e26777f6a5df580e25cb1a63e8f72de3e89eea6ec51733f0e7ca425"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:44:21.269683Z","signature_b64":"S8xje0Gma+hqWsc9Qv2mpD6cG+hAdf62bzJe2KxXU7AFhkyspfRvARlqKbvweKpnZBeIcwlSTJIBRQTxP08MBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8c5d7d930cb2db3c095fb3d7de010ab9d7bbfdc79cce6407973e5ca049c7df92","last_reissued_at":"2026-07-05T07:44:21.269227Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:44:21.269227Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Astrophysical Gravitational Wave Background in the mHz band is likely dominated by White Dwarf binaries","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Gijs Nelemans, Seppe Staelens","submitted_at":"2023-10-30T11:17:56Z","abstract_excerpt":"Context. The Astrophysical Gravitational Wave Background (AGWB) is a collective signal of astrophysical gravitational wave sources and is dominated by compact binaries. Its measurement is one of the science goals of current and future gravitational wave detectors. Aims. We aim to determine what population of compact binaries dominates the AGWB in the mHz band. Methods. We revisit and update earlier work by Farmer & Phinney (2003) to model the astrophysical gravitational wave background sourced by extragalactic white dwarf binaries in the mHz frequency band. We calculate the signal using a sing"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2310.19448","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/2310.19448/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":"2310.19448","created_at":"2026-07-05T07:44:21.269282+00:00"},{"alias_kind":"arxiv_version","alias_value":"2310.19448v3","created_at":"2026-07-05T07:44:21.269282+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2310.19448","created_at":"2026-07-05T07:44:21.269282+00:00"},{"alias_kind":"pith_short_12","alias_value":"RROX3EYMWLNT","created_at":"2026-07-05T07:44:21.269282+00:00"},{"alias_kind":"pith_short_16","alias_value":"RROX3EYMWLNTYCK7","created_at":"2026-07-05T07:44:21.269282+00:00"},{"alias_kind":"pith_short_8","alias_value":"RROX3EYM","created_at":"2026-07-05T07:44:21.269282+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.01992","citing_title":"Reviving Motivated Inflationary Potentials with $K$-inflation in the light of ACT","ref_index":93,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RROX3EYMWLNTYCK7WPL54AIKXH","json":"https://pith.science/pith/RROX3EYMWLNTYCK7WPL54AIKXH.json","graph_json":"https://pith.science/api/pith-number/RROX3EYMWLNTYCK7WPL54AIKXH/graph.json","events_json":"https://pith.science/api/pith-number/RROX3EYMWLNTYCK7WPL54AIKXH/events.json","paper":"https://pith.science/paper/RROX3EYM"},"agent_actions":{"view_html":"https://pith.science/pith/RROX3EYMWLNTYCK7WPL54AIKXH","download_json":"https://pith.science/pith/RROX3EYMWLNTYCK7WPL54AIKXH.json","view_paper":"https://pith.science/paper/RROX3EYM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2310.19448&json=true","fetch_graph":"https://pith.science/api/pith-number/RROX3EYMWLNTYCK7WPL54AIKXH/graph.json","fetch_events":"https://pith.science/api/pith-number/RROX3EYMWLNTYCK7WPL54AIKXH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RROX3EYMWLNTYCK7WPL54AIKXH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RROX3EYMWLNTYCK7WPL54AIKXH/action/storage_attestation","attest_author":"https://pith.science/pith/RROX3EYMWLNTYCK7WPL54AIKXH/action/author_attestation","sign_citation":"https://pith.science/pith/RROX3EYMWLNTYCK7WPL54AIKXH/action/citation_signature","submit_replication":"https://pith.science/pith/RROX3EYMWLNTYCK7WPL54AIKXH/action/replication_record"}},"created_at":"2026-07-05T07:44:21.269282+00:00","updated_at":"2026-07-05T07:44:21.269282+00:00"}