{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:VJAX7A5XQKCAT752W2WSKHFYGU","short_pith_number":"pith:VJAX7A5X","schema_version":"1.0","canonical_sha256":"aa417f83b7828409ffbab6ad251cb8352b209581ba859a1018729841f4b693ad","source":{"kind":"arxiv","id":"2406.11742","version":2},"attestation_state":"computed","paper":{"title":"Detection Prospects of Gravitational Waves from SU(2) Axion Inflation","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Alba Romero-Rodr\\'iguez, Charles Badger, Hannah Duval, Mairi Sakellariadou, Sachiko Kuroyanagi, Tomohiro Fujita","submitted_at":"2024-06-17T17:01:20Z","abstract_excerpt":"We study detection prospects of a gravitational-wave background (GWB) sourced by SU(2) gauge fields considering all possible observational constraints. More precisely, we consider bounds set by cosmic microwave background measurements, primordial black hole overproduction, as well as backreaction of the gauge fields on the background evolution. Gravitational-waves data from the first three observing runs of the LIGO-Virgo-KAGRA Collaboration show no evidence for a GWB contribution from axion inflation. However, we are able to place conservative constraints on the parameters of the SU(2) inflat"},"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":"2406.11742","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-06-17T17:01:20Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"4294bccef6af11a84b74f9f8f1db4d9e72130e447956c51fdf79edebb7fec370","abstract_canon_sha256":"900d2bf01f49bc343d5d3352460b4277dff894d1afaeeb5e1d09d523c605bdea"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:45:29.814158Z","signature_b64":"HVoLtjJwpseIMisODRZxvj8BdY7paHuVlvQlQOR/61RuU6o7UvypU8az06La9c21eSjfR0mQtMa2DY/4dyb9DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"aa417f83b7828409ffbab6ad251cb8352b209581ba859a1018729841f4b693ad","last_reissued_at":"2026-07-05T08:45:29.813738Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:45:29.813738Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detection Prospects of Gravitational Waves from SU(2) Axion Inflation","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Alba Romero-Rodr\\'iguez, Charles Badger, Hannah Duval, Mairi Sakellariadou, Sachiko Kuroyanagi, Tomohiro Fujita","submitted_at":"2024-06-17T17:01:20Z","abstract_excerpt":"We study detection prospects of a gravitational-wave background (GWB) sourced by SU(2) gauge fields considering all possible observational constraints. More precisely, we consider bounds set by cosmic microwave background measurements, primordial black hole overproduction, as well as backreaction of the gauge fields on the background evolution. Gravitational-waves data from the first three observing runs of the LIGO-Virgo-KAGRA Collaboration show no evidence for a GWB contribution from axion inflation. However, we are able to place conservative constraints on the parameters of the SU(2) inflat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2406.11742","kind":"arxiv","version":2},"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/2406.11742/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":"2406.11742","created_at":"2026-07-05T08:45:29.813795+00:00"},{"alias_kind":"arxiv_version","alias_value":"2406.11742v2","created_at":"2026-07-05T08:45:29.813795+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2406.11742","created_at":"2026-07-05T08:45:29.813795+00:00"},{"alias_kind":"pith_short_12","alias_value":"VJAX7A5XQKCA","created_at":"2026-07-05T08:45:29.813795+00:00"},{"alias_kind":"pith_short_16","alias_value":"VJAX7A5XQKCAT752","created_at":"2026-07-05T08:45:29.813795+00:00"},{"alias_kind":"pith_short_8","alias_value":"VJAX7A5X","created_at":"2026-07-05T08:45:29.813795+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/VJAX7A5XQKCAT752W2WSKHFYGU","json":"https://pith.science/pith/VJAX7A5XQKCAT752W2WSKHFYGU.json","graph_json":"https://pith.science/api/pith-number/VJAX7A5XQKCAT752W2WSKHFYGU/graph.json","events_json":"https://pith.science/api/pith-number/VJAX7A5XQKCAT752W2WSKHFYGU/events.json","paper":"https://pith.science/paper/VJAX7A5X"},"agent_actions":{"view_html":"https://pith.science/pith/VJAX7A5XQKCAT752W2WSKHFYGU","download_json":"https://pith.science/pith/VJAX7A5XQKCAT752W2WSKHFYGU.json","view_paper":"https://pith.science/paper/VJAX7A5X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2406.11742&json=true","fetch_graph":"https://pith.science/api/pith-number/VJAX7A5XQKCAT752W2WSKHFYGU/graph.json","fetch_events":"https://pith.science/api/pith-number/VJAX7A5XQKCAT752W2WSKHFYGU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VJAX7A5XQKCAT752W2WSKHFYGU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VJAX7A5XQKCAT752W2WSKHFYGU/action/storage_attestation","attest_author":"https://pith.science/pith/VJAX7A5XQKCAT752W2WSKHFYGU/action/author_attestation","sign_citation":"https://pith.science/pith/VJAX7A5XQKCAT752W2WSKHFYGU/action/citation_signature","submit_replication":"https://pith.science/pith/VJAX7A5XQKCAT752W2WSKHFYGU/action/replication_record"}},"created_at":"2026-07-05T08:45:29.813795+00:00","updated_at":"2026-07-05T08:45:29.813795+00:00"}