{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:3O72S7IGHJSJUVHB2ZSXTE6OX4","short_pith_number":"pith:3O72S7IG","schema_version":"1.0","canonical_sha256":"dbbfa97d063a649a54e1d6657993cebf3abaa36e6effd39c4426751db2eb9bb8","source":{"kind":"arxiv","id":"2211.14465","version":2},"attestation_state":"computed","paper":{"title":"Effective Chiral Magnetic Effect from Neutrino Radiation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","nucl-th"],"primary_cat":"hep-ph","authors_text":"Di-Lun Yang, Naoki Yamamoto","submitted_at":"2022-11-26T03:12:38Z","abstract_excerpt":"We develop an approach to chiral kinetic theories for electrons close to equilibrium and neutrinos away from equilibrium based on a systematic power counting scheme for different timescales of electromagnetic and weak interactions. Under this framework, we derive electric and energy currents along magnetic fields induced by neutrino radiation in general nonequilibrium states. This may be regarded as an effective chiral magnetic effect (CME), which is present without a chiral chemical potential, unlike the conventional CME. We also consider the so-called gain region of core-collapse supernovae "},"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":"2211.14465","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2022-11-26T03:12:38Z","cross_cats_sorted":["astro-ph.HE","nucl-th"],"title_canon_sha256":"e1ae87e9fa62301bcb3b498a14a8832213238814580216f90e3ef2ede0aabb41","abstract_canon_sha256":"6040300b75f01a62c9696a1e39db3b8dece1e6b00681c34e3068b12d43674cc4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:28:57.254533Z","signature_b64":"4wtbv3FtP1yGDL/pp4L+IyuOBc9tYPL/1fdeg0Ehc5WIR9hFEOKeEunh348hDtb/Di9lGhAmKducBfVXF6ItBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dbbfa97d063a649a54e1d6657993cebf3abaa36e6effd39c4426751db2eb9bb8","last_reissued_at":"2026-07-05T06:28:57.254083Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:28:57.254083Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Effective Chiral Magnetic Effect from Neutrino Radiation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","nucl-th"],"primary_cat":"hep-ph","authors_text":"Di-Lun Yang, Naoki Yamamoto","submitted_at":"2022-11-26T03:12:38Z","abstract_excerpt":"We develop an approach to chiral kinetic theories for electrons close to equilibrium and neutrinos away from equilibrium based on a systematic power counting scheme for different timescales of electromagnetic and weak interactions. Under this framework, we derive electric and energy currents along magnetic fields induced by neutrino radiation in general nonequilibrium states. This may be regarded as an effective chiral magnetic effect (CME), which is present without a chiral chemical potential, unlike the conventional CME. We also consider the so-called gain region of core-collapse supernovae "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2211.14465","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/2211.14465/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":"2211.14465","created_at":"2026-07-05T06:28:57.254139+00:00"},{"alias_kind":"arxiv_version","alias_value":"2211.14465v2","created_at":"2026-07-05T06:28:57.254139+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2211.14465","created_at":"2026-07-05T06:28:57.254139+00:00"},{"alias_kind":"pith_short_12","alias_value":"3O72S7IGHJSJ","created_at":"2026-07-05T06:28:57.254139+00:00"},{"alias_kind":"pith_short_16","alias_value":"3O72S7IGHJSJUVHB","created_at":"2026-07-05T06:28:57.254139+00:00"},{"alias_kind":"pith_short_8","alias_value":"3O72S7IG","created_at":"2026-07-05T06:28:57.254139+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2510.00114","citing_title":"Chiral effects and Joule heating in hot and dense matter","ref_index":23,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3O72S7IGHJSJUVHB2ZSXTE6OX4","json":"https://pith.science/pith/3O72S7IGHJSJUVHB2ZSXTE6OX4.json","graph_json":"https://pith.science/api/pith-number/3O72S7IGHJSJUVHB2ZSXTE6OX4/graph.json","events_json":"https://pith.science/api/pith-number/3O72S7IGHJSJUVHB2ZSXTE6OX4/events.json","paper":"https://pith.science/paper/3O72S7IG"},"agent_actions":{"view_html":"https://pith.science/pith/3O72S7IGHJSJUVHB2ZSXTE6OX4","download_json":"https://pith.science/pith/3O72S7IGHJSJUVHB2ZSXTE6OX4.json","view_paper":"https://pith.science/paper/3O72S7IG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2211.14465&json=true","fetch_graph":"https://pith.science/api/pith-number/3O72S7IGHJSJUVHB2ZSXTE6OX4/graph.json","fetch_events":"https://pith.science/api/pith-number/3O72S7IGHJSJUVHB2ZSXTE6OX4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3O72S7IGHJSJUVHB2ZSXTE6OX4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3O72S7IGHJSJUVHB2ZSXTE6OX4/action/storage_attestation","attest_author":"https://pith.science/pith/3O72S7IGHJSJUVHB2ZSXTE6OX4/action/author_attestation","sign_citation":"https://pith.science/pith/3O72S7IGHJSJUVHB2ZSXTE6OX4/action/citation_signature","submit_replication":"https://pith.science/pith/3O72S7IGHJSJUVHB2ZSXTE6OX4/action/replication_record"}},"created_at":"2026-07-05T06:28:57.254139+00:00","updated_at":"2026-07-05T06:28:57.254139+00:00"}