{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1997:2SSEC5UWW5NNRVGA3FJ3CBIRDJ","short_pith_number":"pith:2SSEC5UW","schema_version":"1.0","canonical_sha256":"d4a4417696b75ad8d4c0d953b105111a440cc4272e84ecaac32109de547d8d9b","source":{"kind":"arxiv","id":"hep-ph/9703214","version":2},"attestation_state":"computed","paper":{"title":"Neutrinos with Magnetic Moment: Depolarization Rate in Plasma","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"hep-ph","authors_text":"Georg Raffelt (M\\\"unich), G\\\"unter Sigl (Chicago), Kari Enqvist (Helsinki), Per Elmfors (Stockholm)","submitted_at":"1997-03-03T09:20:53Z","abstract_excerpt":"Neutrinos with a magnetic moment $\\mu$ change their helicity when interacting with an electromagnetic field. Various aspects of this effect have been described as spin precession, spin-flip scattering, and magnetic Cherenkov radiation. These perspectives are unified in an expression for the $\\nu_L\\to\\nu_R$ transition rate which involves the correlators of the electromagnetic field distribution. Our general formula corrects a previous result and generalizes it to the case where the fields cannot be viewed as classical and where the momentum transfers need not be small. We evaluate our result ex"},"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":"hep-ph/9703214","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"1997-03-03T09:20:53Z","cross_cats_sorted":["astro-ph"],"title_canon_sha256":"2c6797a6fd718b6a2f3d51a1380a9fc7dbbeb29fca683f7c1a4dbe1037c7b668","abstract_canon_sha256":"deedb08a768d110996fe891d65702d2d8f27f59c633a6d00f4d257a0f787b0bc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:18:23.082771Z","signature_b64":"qVFKNnZOhGG5nb1phDT7iopJji4Dp4u9fhCcJwfTq5oVshcUWIGyIa2LRMSB8PWPsOFlbpNzeKxlRTBCVg+oCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d4a4417696b75ad8d4c0d953b105111a440cc4272e84ecaac32109de547d8d9b","last_reissued_at":"2026-07-04T15:18:23.082338Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:18:23.082338Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutrinos with Magnetic Moment: Depolarization Rate in Plasma","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"hep-ph","authors_text":"Georg Raffelt (M\\\"unich), G\\\"unter Sigl (Chicago), Kari Enqvist (Helsinki), Per Elmfors (Stockholm)","submitted_at":"1997-03-03T09:20:53Z","abstract_excerpt":"Neutrinos with a magnetic moment $\\mu$ change their helicity when interacting with an electromagnetic field. Various aspects of this effect have been described as spin precession, spin-flip scattering, and magnetic Cherenkov radiation. These perspectives are unified in an expression for the $\\nu_L\\to\\nu_R$ transition rate which involves the correlators of the electromagnetic field distribution. Our general formula corrects a previous result and generalizes it to the case where the fields cannot be viewed as classical and where the momentum transfers need not be small. We evaluate our result ex"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9703214","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/hep-ph/9703214/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":"hep-ph/9703214","created_at":"2026-07-04T15:18:23.082388+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/9703214v2","created_at":"2026-07-04T15:18:23.082388+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/9703214","created_at":"2026-07-04T15:18:23.082388+00:00"},{"alias_kind":"pith_short_12","alias_value":"2SSEC5UWW5NN","created_at":"2026-07-04T15:18:23.082388+00:00"},{"alias_kind":"pith_short_16","alias_value":"2SSEC5UWW5NNRVGA","created_at":"2026-07-04T15:18:23.082388+00:00"},{"alias_kind":"pith_short_8","alias_value":"2SSEC5UW","created_at":"2026-07-04T15:18:23.082388+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2604.06493","citing_title":"Low-Scale Leptogenesis from Resonant Thermal Lepton Flavour Coherences","ref_index":58,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2SSEC5UWW5NNRVGA3FJ3CBIRDJ","json":"https://pith.science/pith/2SSEC5UWW5NNRVGA3FJ3CBIRDJ.json","graph_json":"https://pith.science/api/pith-number/2SSEC5UWW5NNRVGA3FJ3CBIRDJ/graph.json","events_json":"https://pith.science/api/pith-number/2SSEC5UWW5NNRVGA3FJ3CBIRDJ/events.json","paper":"https://pith.science/paper/2SSEC5UW"},"agent_actions":{"view_html":"https://pith.science/pith/2SSEC5UWW5NNRVGA3FJ3CBIRDJ","download_json":"https://pith.science/pith/2SSEC5UWW5NNRVGA3FJ3CBIRDJ.json","view_paper":"https://pith.science/paper/2SSEC5UW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/9703214&json=true","fetch_graph":"https://pith.science/api/pith-number/2SSEC5UWW5NNRVGA3FJ3CBIRDJ/graph.json","fetch_events":"https://pith.science/api/pith-number/2SSEC5UWW5NNRVGA3FJ3CBIRDJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2SSEC5UWW5NNRVGA3FJ3CBIRDJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2SSEC5UWW5NNRVGA3FJ3CBIRDJ/action/storage_attestation","attest_author":"https://pith.science/pith/2SSEC5UWW5NNRVGA3FJ3CBIRDJ/action/author_attestation","sign_citation":"https://pith.science/pith/2SSEC5UWW5NNRVGA3FJ3CBIRDJ/action/citation_signature","submit_replication":"https://pith.science/pith/2SSEC5UWW5NNRVGA3FJ3CBIRDJ/action/replication_record"}},"created_at":"2026-07-04T15:18:23.082388+00:00","updated_at":"2026-07-04T15:18:23.082388+00:00"}