{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:F67J7KWHFK7JMOWW76IVVOXX5K","short_pith_number":"pith:F67J7KWH","schema_version":"1.0","canonical_sha256":"2fbe9faac72abe963ad6ff915abaf7eab52a34d61d08a12e0bdb4d85978a59d7","source":{"kind":"arxiv","id":"2210.06481","version":2},"attestation_state":"computed","paper":{"title":"On the Sensitivity of Spin-Precession Axion Experiments","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"Jacob M. Leedom, Jeff A. Dror, Nicholas L. Rodd, Stefania Gori","submitted_at":"2022-10-12T18:00:00Z","abstract_excerpt":"A leading direction in the hunt for axion dark matter is to search for its influence on nuclear spins. The detection scheme involves polarizing a sample of nuclei within a strong static magnetic field and then looking for a spin precession induced by the oscillating axion field. We study the axion signal and background contributions that arise in such experiments (a prominent example being CASPEr), finding key differences with the existing literature. Most importantly, in the limit where the transverse spin-relaxation time of the material is the largest timescale of the problem, we show that t"},"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":"2210.06481","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2022-10-12T18:00:00Z","cross_cats_sorted":["astro-ph.CO","hep-ex"],"title_canon_sha256":"2064bdc139652a30debead24a691f596a09e2cebf078b43b6869a65cfcbeb08f","abstract_canon_sha256":"81721038d6ced80d48c8cec43d5acd5a7313f5cd4d7e4fdcf67c9e032b4da73f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:09:31.949637Z","signature_b64":"+ARmAC0yFNGHDd3Cr2X10NhTtYbVk9Ff+6LoaYaG+AVThKoHM5bxLqR1H1MrOgDzh2TvcrpIB3L4XME8w6pFCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2fbe9faac72abe963ad6ff915abaf7eab52a34d61d08a12e0bdb4d85978a59d7","last_reissued_at":"2026-07-05T06:09:31.949181Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:09:31.949181Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the Sensitivity of Spin-Precession Axion Experiments","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"Jacob M. Leedom, Jeff A. Dror, Nicholas L. Rodd, Stefania Gori","submitted_at":"2022-10-12T18:00:00Z","abstract_excerpt":"A leading direction in the hunt for axion dark matter is to search for its influence on nuclear spins. The detection scheme involves polarizing a sample of nuclei within a strong static magnetic field and then looking for a spin precession induced by the oscillating axion field. We study the axion signal and background contributions that arise in such experiments (a prominent example being CASPEr), finding key differences with the existing literature. Most importantly, in the limit where the transverse spin-relaxation time of the material is the largest timescale of the problem, we show that t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2210.06481","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/2210.06481/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":"2210.06481","created_at":"2026-07-05T06:09:31.949246+00:00"},{"alias_kind":"arxiv_version","alias_value":"2210.06481v2","created_at":"2026-07-05T06:09:31.949246+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2210.06481","created_at":"2026-07-05T06:09:31.949246+00:00"},{"alias_kind":"pith_short_12","alias_value":"F67J7KWHFK7J","created_at":"2026-07-05T06:09:31.949246+00:00"},{"alias_kind":"pith_short_16","alias_value":"F67J7KWHFK7JMOWW","created_at":"2026-07-05T06:09:31.949246+00:00"},{"alias_kind":"pith_short_8","alias_value":"F67J7KWH","created_at":"2026-07-05T06:09:31.949246+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.09982","citing_title":"Testing F-theory GUTs with the Axiverse","ref_index":189,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/F67J7KWHFK7JMOWW76IVVOXX5K","json":"https://pith.science/pith/F67J7KWHFK7JMOWW76IVVOXX5K.json","graph_json":"https://pith.science/api/pith-number/F67J7KWHFK7JMOWW76IVVOXX5K/graph.json","events_json":"https://pith.science/api/pith-number/F67J7KWHFK7JMOWW76IVVOXX5K/events.json","paper":"https://pith.science/paper/F67J7KWH"},"agent_actions":{"view_html":"https://pith.science/pith/F67J7KWHFK7JMOWW76IVVOXX5K","download_json":"https://pith.science/pith/F67J7KWHFK7JMOWW76IVVOXX5K.json","view_paper":"https://pith.science/paper/F67J7KWH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2210.06481&json=true","fetch_graph":"https://pith.science/api/pith-number/F67J7KWHFK7JMOWW76IVVOXX5K/graph.json","fetch_events":"https://pith.science/api/pith-number/F67J7KWHFK7JMOWW76IVVOXX5K/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/F67J7KWHFK7JMOWW76IVVOXX5K/action/timestamp_anchor","attest_storage":"https://pith.science/pith/F67J7KWHFK7JMOWW76IVVOXX5K/action/storage_attestation","attest_author":"https://pith.science/pith/F67J7KWHFK7JMOWW76IVVOXX5K/action/author_attestation","sign_citation":"https://pith.science/pith/F67J7KWHFK7JMOWW76IVVOXX5K/action/citation_signature","submit_replication":"https://pith.science/pith/F67J7KWHFK7JMOWW76IVVOXX5K/action/replication_record"}},"created_at":"2026-07-05T06:09:31.949246+00:00","updated_at":"2026-07-05T06:09:31.949246+00:00"}