{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:O7ZROIDCGGXVKRFPKQAI43OLFV","short_pith_number":"pith:O7ZROIDC","schema_version":"1.0","canonical_sha256":"77f317206231af5544af54008e6dcb2d64f14edc5c4316c8c066e94e2b809120","source":{"kind":"arxiv","id":"hep-ph/0403168","version":1},"attestation_state":"computed","paper":{"title":"Neutrino-Electron Scattering Theory","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"William J. Marciano, Zohreh Parsa","submitted_at":"2004-03-15T22:27:21Z","abstract_excerpt":"Standard Model predictions for neutrino-electron scattering cross-sections, including effects of electroweak radiative corrections, are reviewed. The sensitivity of those quantities to neutrino dipole moments, z' bosons, dynamical symmetry breaking and other types of ``New Physics'' is described. Neutrino indices of refraction in matter are also discussed. A perspective on future initiatives with intense neutrino sources, such as superbeams and neutrino factories, is given."},"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/0403168","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2004-03-15T22:27:21Z","cross_cats_sorted":[],"title_canon_sha256":"f68b9034705c6890eb1b5401402f72e60d900edbc307da03295b5de4d6644e0a","abstract_canon_sha256":"99cef40d04fe4e061f181e72c41d83035fb0bea0213242b55afe045979861bd7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:20:23.462281Z","signature_b64":"JpKP81gY7vwNgfR7Ejq4VD/j0wTCmdDWBmOtD7eMMumAFj8ggz5mUma0CP5slfxm6hT8B5VlCabfkxAvGvVpCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"77f317206231af5544af54008e6dcb2d64f14edc5c4316c8c066e94e2b809120","last_reissued_at":"2026-07-04T15:20:23.461802Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:20:23.461802Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutrino-Electron Scattering Theory","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"William J. Marciano, Zohreh Parsa","submitted_at":"2004-03-15T22:27:21Z","abstract_excerpt":"Standard Model predictions for neutrino-electron scattering cross-sections, including effects of electroweak radiative corrections, are reviewed. The sensitivity of those quantities to neutrino dipole moments, z' bosons, dynamical symmetry breaking and other types of ``New Physics'' is described. Neutrino indices of refraction in matter are also discussed. A perspective on future initiatives with intense neutrino sources, such as superbeams and neutrino factories, is given."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0403168","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/hep-ph/0403168/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/0403168","created_at":"2026-07-04T15:20:23.461856+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0403168v1","created_at":"2026-07-04T15:20:23.461856+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0403168","created_at":"2026-07-04T15:20:23.461856+00:00"},{"alias_kind":"pith_short_12","alias_value":"O7ZROIDCGGXV","created_at":"2026-07-04T15:20:23.461856+00:00"},{"alias_kind":"pith_short_16","alias_value":"O7ZROIDCGGXVKRFP","created_at":"2026-07-04T15:20:23.461856+00:00"},{"alias_kind":"pith_short_8","alias_value":"O7ZROIDC","created_at":"2026-07-04T15:20:23.461856+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2606.30756","citing_title":"Parameterizing the Standing Accretion Shock Instability for Inference with Galactic Supernova Neutrino Signals at IceCube","ref_index":83,"is_internal_anchor":true},{"citing_arxiv_id":"2605.28671","citing_title":"CP-violation or Nuclear Excitation: Reviewing the Role of Neutrino Interaction Model Uncertainties on Accelerator-Based Neutrino Oscillation Measurements","ref_index":250,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/O7ZROIDCGGXVKRFPKQAI43OLFV","json":"https://pith.science/pith/O7ZROIDCGGXVKRFPKQAI43OLFV.json","graph_json":"https://pith.science/api/pith-number/O7ZROIDCGGXVKRFPKQAI43OLFV/graph.json","events_json":"https://pith.science/api/pith-number/O7ZROIDCGGXVKRFPKQAI43OLFV/events.json","paper":"https://pith.science/paper/O7ZROIDC"},"agent_actions":{"view_html":"https://pith.science/pith/O7ZROIDCGGXVKRFPKQAI43OLFV","download_json":"https://pith.science/pith/O7ZROIDCGGXVKRFPKQAI43OLFV.json","view_paper":"https://pith.science/paper/O7ZROIDC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0403168&json=true","fetch_graph":"https://pith.science/api/pith-number/O7ZROIDCGGXVKRFPKQAI43OLFV/graph.json","fetch_events":"https://pith.science/api/pith-number/O7ZROIDCGGXVKRFPKQAI43OLFV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/O7ZROIDCGGXVKRFPKQAI43OLFV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/O7ZROIDCGGXVKRFPKQAI43OLFV/action/storage_attestation","attest_author":"https://pith.science/pith/O7ZROIDCGGXVKRFPKQAI43OLFV/action/author_attestation","sign_citation":"https://pith.science/pith/O7ZROIDCGGXVKRFPKQAI43OLFV/action/citation_signature","submit_replication":"https://pith.science/pith/O7ZROIDCGGXVKRFPKQAI43OLFV/action/replication_record"}},"created_at":"2026-07-04T15:20:23.461856+00:00","updated_at":"2026-07-04T15:20:23.461856+00:00"}