{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:CSYXFYKG2QQSLUO2CKQHHZAAXF","short_pith_number":"pith:CSYXFYKG","schema_version":"1.0","canonical_sha256":"14b172e146d42125d1da12a073e400b97c330bda56783c6694cbebbc779711c3","source":{"kind":"arxiv","id":"2009.07733","version":2},"attestation_state":"computed","paper":{"title":"Impact of magnetic field on neutrino-matter interactions in core-collapse supernova","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Takami Kuroda","submitted_at":"2020-09-16T15:06:33Z","abstract_excerpt":"We explore the impact of magnetic field on neutrino-matter interactions in core-collapse supernova. We first derive the modified source terms for neutrino-nucleon scattering and neutrino absorption and emission processes in the moment formalism. Then we perform full relativistic three-dimensional, magnetorotational core-collapse supernova simulations of a 20 $M_\\odot$ star with spectral neutrino transport. Our simulations treat self-consistently the parity violation effects of weak interaction in the presence of external magnetic field. The result shows a significant global asymmetry, mostly c"},"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":"2009.07733","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-09-16T15:06:33Z","cross_cats_sorted":[],"title_canon_sha256":"aaebbd2462f5a34379b1f8f3d5b63cc3978a524b9fa71863610cc43e076e5b42","abstract_canon_sha256":"17a08002e8b28d5ee72285d42ddc65cde47cd8443dee7addbc5d815c614da569"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:09:46.741864Z","signature_b64":"h0T58EEQZtJ0MEYIdFIHcdZdODwan02slyLqkVoIYG5edAS7No6onYFfFbwWpT1JmBNPOB6bLgc8vDlNreL7AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"14b172e146d42125d1da12a073e400b97c330bda56783c6694cbebbc779711c3","last_reissued_at":"2026-07-05T02:09:46.741486Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:09:46.741486Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Impact of magnetic field on neutrino-matter interactions in core-collapse supernova","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Takami Kuroda","submitted_at":"2020-09-16T15:06:33Z","abstract_excerpt":"We explore the impact of magnetic field on neutrino-matter interactions in core-collapse supernova. We first derive the modified source terms for neutrino-nucleon scattering and neutrino absorption and emission processes in the moment formalism. Then we perform full relativistic three-dimensional, magnetorotational core-collapse supernova simulations of a 20 $M_\\odot$ star with spectral neutrino transport. Our simulations treat self-consistently the parity violation effects of weak interaction in the presence of external magnetic field. The result shows a significant global asymmetry, mostly c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2009.07733","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/2009.07733/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":"2009.07733","created_at":"2026-07-05T02:09:46.741539+00:00"},{"alias_kind":"arxiv_version","alias_value":"2009.07733v2","created_at":"2026-07-05T02:09:46.741539+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2009.07733","created_at":"2026-07-05T02:09:46.741539+00:00"},{"alias_kind":"pith_short_12","alias_value":"CSYXFYKG2QQS","created_at":"2026-07-05T02:09:46.741539+00:00"},{"alias_kind":"pith_short_16","alias_value":"CSYXFYKG2QQSLUO2","created_at":"2026-07-05T02:09:46.741539+00:00"},{"alias_kind":"pith_short_8","alias_value":"CSYXFYKG","created_at":"2026-07-05T02:09:46.741539+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06664","citing_title":"Effects of Rotation on 3D Core-Collapse Supernova Models for Low-Mass Progenitors","ref_index":291,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CSYXFYKG2QQSLUO2CKQHHZAAXF","json":"https://pith.science/pith/CSYXFYKG2QQSLUO2CKQHHZAAXF.json","graph_json":"https://pith.science/api/pith-number/CSYXFYKG2QQSLUO2CKQHHZAAXF/graph.json","events_json":"https://pith.science/api/pith-number/CSYXFYKG2QQSLUO2CKQHHZAAXF/events.json","paper":"https://pith.science/paper/CSYXFYKG"},"agent_actions":{"view_html":"https://pith.science/pith/CSYXFYKG2QQSLUO2CKQHHZAAXF","download_json":"https://pith.science/pith/CSYXFYKG2QQSLUO2CKQHHZAAXF.json","view_paper":"https://pith.science/paper/CSYXFYKG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2009.07733&json=true","fetch_graph":"https://pith.science/api/pith-number/CSYXFYKG2QQSLUO2CKQHHZAAXF/graph.json","fetch_events":"https://pith.science/api/pith-number/CSYXFYKG2QQSLUO2CKQHHZAAXF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CSYXFYKG2QQSLUO2CKQHHZAAXF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CSYXFYKG2QQSLUO2CKQHHZAAXF/action/storage_attestation","attest_author":"https://pith.science/pith/CSYXFYKG2QQSLUO2CKQHHZAAXF/action/author_attestation","sign_citation":"https://pith.science/pith/CSYXFYKG2QQSLUO2CKQHHZAAXF/action/citation_signature","submit_replication":"https://pith.science/pith/CSYXFYKG2QQSLUO2CKQHHZAAXF/action/replication_record"}},"created_at":"2026-07-05T02:09:46.741539+00:00","updated_at":"2026-07-05T02:09:46.741539+00:00"}