{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1998:QJ7PEQ6YWEDLDTYL6RIKQK7TYH","short_pith_number":"pith:QJ7PEQ6Y","schema_version":"1.0","canonical_sha256":"827ef243d8b106b1cf0bf450a82bf3c1ef219d13560794eaa294de0c98d4340c","source":{"kind":"arxiv","id":"nucl-th/9808047","version":1},"attestation_state":"computed","paper":{"title":"Magnetic Radius of the Deuteron","license":"","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"Andrei V. Afanasev, S.V. Trubnikov, V.D. Afanasev","submitted_at":"1998-08-17T18:38:08Z","abstract_excerpt":"The root-mean square radius of the deuteron magnetic moment distribution, $ r_{Md}$, is calculated for several realistic models of the $NN$--interaction. For the Paris potential the result is $r_{Md} = 2.312 \\pm 0.010 $ fm. The dependence of $r_{Md} $ on the choice of $NN$ model, relativistic effects and meson exchange currents is investigated. The experimental value of $r_{Md}$ is also considered. The necessity of new precise measurements of the deuteron magnetic form factor at low values of $Q^2$ is stressed."},"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":"nucl-th/9808047","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"nucl-th","submitted_at":"1998-08-17T18:38:08Z","cross_cats_sorted":[],"title_canon_sha256":"bd687ad12d3949ebb03c428ba57f06d53b4182da836b08e82e2392540050c292","abstract_canon_sha256":"7c76bc210d54c9b15ae2db0ceef0575271864220e51e3f73c071b350e55ae5ce"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T14:42:58.964888Z","signature_b64":"/pxCcoAHVdQZzWZT4Jb/2GZI5gBc8c6U4h0LJ/MUuU14zVT22AuIePuAVfEKwxOz4VaZBGy7c+ty5bRuF1zRDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"827ef243d8b106b1cf0bf450a82bf3c1ef219d13560794eaa294de0c98d4340c","last_reissued_at":"2026-07-04T14:42:58.964485Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T14:42:58.964485Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Magnetic Radius of the Deuteron","license":"","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"Andrei V. Afanasev, S.V. Trubnikov, V.D. Afanasev","submitted_at":"1998-08-17T18:38:08Z","abstract_excerpt":"The root-mean square radius of the deuteron magnetic moment distribution, $ r_{Md}$, is calculated for several realistic models of the $NN$--interaction. For the Paris potential the result is $r_{Md} = 2.312 \\pm 0.010 $ fm. The dependence of $r_{Md} $ on the choice of $NN$ model, relativistic effects and meson exchange currents is investigated. The experimental value of $r_{Md}$ is also considered. The necessity of new precise measurements of the deuteron magnetic form factor at low values of $Q^2$ is stressed."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"nucl-th/9808047","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/nucl-th/9808047/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":"nucl-th/9808047","created_at":"2026-07-04T14:42:58.964547+00:00"},{"alias_kind":"arxiv_version","alias_value":"nucl-th/9808047v1","created_at":"2026-07-04T14:42:58.964547+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.nucl-th/9808047","created_at":"2026-07-04T14:42:58.964547+00:00"},{"alias_kind":"pith_short_12","alias_value":"QJ7PEQ6YWEDL","created_at":"2026-07-04T14:42:58.964547+00:00"},{"alias_kind":"pith_short_16","alias_value":"QJ7PEQ6YWEDLDTYL","created_at":"2026-07-04T14:42:58.964547+00:00"},{"alias_kind":"pith_short_8","alias_value":"QJ7PEQ6Y","created_at":"2026-07-04T14:42:58.964547+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.09886","citing_title":"Structure of lightest nuclei in the visible Universe","ref_index":59,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QJ7PEQ6YWEDLDTYL6RIKQK7TYH","json":"https://pith.science/pith/QJ7PEQ6YWEDLDTYL6RIKQK7TYH.json","graph_json":"https://pith.science/api/pith-number/QJ7PEQ6YWEDLDTYL6RIKQK7TYH/graph.json","events_json":"https://pith.science/api/pith-number/QJ7PEQ6YWEDLDTYL6RIKQK7TYH/events.json","paper":"https://pith.science/paper/QJ7PEQ6Y"},"agent_actions":{"view_html":"https://pith.science/pith/QJ7PEQ6YWEDLDTYL6RIKQK7TYH","download_json":"https://pith.science/pith/QJ7PEQ6YWEDLDTYL6RIKQK7TYH.json","view_paper":"https://pith.science/paper/QJ7PEQ6Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=nucl-th/9808047&json=true","fetch_graph":"https://pith.science/api/pith-number/QJ7PEQ6YWEDLDTYL6RIKQK7TYH/graph.json","fetch_events":"https://pith.science/api/pith-number/QJ7PEQ6YWEDLDTYL6RIKQK7TYH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QJ7PEQ6YWEDLDTYL6RIKQK7TYH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QJ7PEQ6YWEDLDTYL6RIKQK7TYH/action/storage_attestation","attest_author":"https://pith.science/pith/QJ7PEQ6YWEDLDTYL6RIKQK7TYH/action/author_attestation","sign_citation":"https://pith.science/pith/QJ7PEQ6YWEDLDTYL6RIKQK7TYH/action/citation_signature","submit_replication":"https://pith.science/pith/QJ7PEQ6YWEDLDTYL6RIKQK7TYH/action/replication_record"}},"created_at":"2026-07-04T14:42:58.964547+00:00","updated_at":"2026-07-04T14:42:58.964547+00:00"}