{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:JIKGAZPARHCCFVFL3YEHIIUVVR","short_pith_number":"pith:JIKGAZPA","schema_version":"1.0","canonical_sha256":"4a146065e089c422d4abde08742295ac461fe958409f7add36767ef998549063","source":{"kind":"arxiv","id":"2411.19441","version":2},"attestation_state":"computed","paper":{"title":"Indirect detection of the QCD axion","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Bradley J. Kavanagh, Bradley Johnson, David J.E. Marsh, Jordan E. Shroyer, Liam Walters, Luca Visinelli","submitted_at":"2024-11-29T02:53:27Z","abstract_excerpt":"The QCD axion, originally proposed to solve the strong CP problem in QCD, is a prominent candidate for dark matter (DM). In the presence of strong magnetic fields, such as those around neutron stars, axions can theoretically convert into photons, producing detectable electromagnetic signals. This axion-photon coupling provides a unique experimental pathway to probe axions within a specific mass range. We investigate a novel observational approach using the Green Bank Telescope (GBT) to search for radio transients that could arise from interactions between neutron stars and dense DM clumps know"},"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":"2411.19441","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-11-29T02:53:27Z","cross_cats_sorted":["hep-ph","hep-th"],"title_canon_sha256":"6374598083b786b2064fb382629c03b41006470ec87b173cc3ab7c787bcf0a08","abstract_canon_sha256":"e6535b23aff4a4bd5b62ce73e307b31a449c22ec0e2c38ee8eaceb02a9b121cf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:16:17.373220Z","signature_b64":"FDqJzhUpy+8pFcer2tzWQNgtq0Q3c7kP6pu+XtP8RD5OnKX3vWcWW/p+YvPnr7m7MmC6wLIMqoN28wlYm3ATAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4a146065e089c422d4abde08742295ac461fe958409f7add36767ef998549063","last_reissued_at":"2026-07-05T10:16:17.372669Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:16:17.372669Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Indirect detection of the QCD axion","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Bradley J. Kavanagh, Bradley Johnson, David J.E. Marsh, Jordan E. Shroyer, Liam Walters, Luca Visinelli","submitted_at":"2024-11-29T02:53:27Z","abstract_excerpt":"The QCD axion, originally proposed to solve the strong CP problem in QCD, is a prominent candidate for dark matter (DM). In the presence of strong magnetic fields, such as those around neutron stars, axions can theoretically convert into photons, producing detectable electromagnetic signals. This axion-photon coupling provides a unique experimental pathway to probe axions within a specific mass range. We investigate a novel observational approach using the Green Bank Telescope (GBT) to search for radio transients that could arise from interactions between neutron stars and dense DM clumps know"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.19441","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/2411.19441/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":"2411.19441","created_at":"2026-07-05T10:16:17.372740+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.19441v2","created_at":"2026-07-05T10:16:17.372740+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.19441","created_at":"2026-07-05T10:16:17.372740+00:00"},{"alias_kind":"pith_short_12","alias_value":"JIKGAZPARHCC","created_at":"2026-07-05T10:16:17.372740+00:00"},{"alias_kind":"pith_short_16","alias_value":"JIKGAZPARHCCFVFL","created_at":"2026-07-05T10:16:17.372740+00:00"},{"alias_kind":"pith_short_8","alias_value":"JIKGAZPA","created_at":"2026-07-05T10:16:17.372740+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.19439","citing_title":"From Rags to Jeans: Axion Miniclusters from Early matter domination","ref_index":100,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JIKGAZPARHCCFVFL3YEHIIUVVR","json":"https://pith.science/pith/JIKGAZPARHCCFVFL3YEHIIUVVR.json","graph_json":"https://pith.science/api/pith-number/JIKGAZPARHCCFVFL3YEHIIUVVR/graph.json","events_json":"https://pith.science/api/pith-number/JIKGAZPARHCCFVFL3YEHIIUVVR/events.json","paper":"https://pith.science/paper/JIKGAZPA"},"agent_actions":{"view_html":"https://pith.science/pith/JIKGAZPARHCCFVFL3YEHIIUVVR","download_json":"https://pith.science/pith/JIKGAZPARHCCFVFL3YEHIIUVVR.json","view_paper":"https://pith.science/paper/JIKGAZPA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.19441&json=true","fetch_graph":"https://pith.science/api/pith-number/JIKGAZPARHCCFVFL3YEHIIUVVR/graph.json","fetch_events":"https://pith.science/api/pith-number/JIKGAZPARHCCFVFL3YEHIIUVVR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JIKGAZPARHCCFVFL3YEHIIUVVR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JIKGAZPARHCCFVFL3YEHIIUVVR/action/storage_attestation","attest_author":"https://pith.science/pith/JIKGAZPARHCCFVFL3YEHIIUVVR/action/author_attestation","sign_citation":"https://pith.science/pith/JIKGAZPARHCCFVFL3YEHIIUVVR/action/citation_signature","submit_replication":"https://pith.science/pith/JIKGAZPARHCCFVFL3YEHIIUVVR/action/replication_record"}},"created_at":"2026-07-05T10:16:17.372740+00:00","updated_at":"2026-07-05T10:16:17.372740+00:00"}