{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:VXXQUDLAPOPKFLDAARHAHM6ET5","short_pith_number":"pith:VXXQUDLA","schema_version":"1.0","canonical_sha256":"adef0a0d607b9ea2ac60044e03b3c49f48f0469c1ace385ba7fd21a03d4bc517","source":{"kind":"arxiv","id":"1012.1339","version":2},"attestation_state":"computed","paper":{"title":"Multi-angle effects in self-induced oscillations for different supernova neutrino fluxes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"hep-ph","authors_text":"Alessandro Mirizzi (Hamburg U., II Inst. Theor. Phys.), Ricard Tom\\`as (Hamburg U.","submitted_at":"2010-12-06T21:17:07Z","abstract_excerpt":"The non-isotropic nature of the neutrino emission from a supernova (SN) core might potentially affect the flavor evolution of the neutrino ensemble, via neutrino-neutrino interactions in the deepest SN regions. We investigate the dependence of these \"multi-angle effects\" on the original SN neutrino fluxes in a three-flavor framework. We show that the pattern of the spectral crossings (energies where F_\\nu_e= F_\\nu_x, and F_\\bar\\nu_e= F_\\bar\\nu_x) is crucial in determining the impact of multi-angle effects on the flavor evolution. For neutrino spectra presenting only a single-crossing, synchron"},"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":"1012.1339","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-12-06T21:17:07Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"77a2f99629f0b1785d751e306c0f705fadeaa9dae17b7157c47e9f5f49b142ff","abstract_canon_sha256":"2790b71f0ff6bae08d309d3308c0f7705f076083c502ed8d38d70a0200956898"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:23:14.980628Z","signature_b64":"HpmpEXsg4h6CL3Qyi3iLZgjuowUqKNTn49ZJXlex/RvtlzMpfuav8DrU1ZIPIYz8zsUfI5yWuHctpmn60UrHBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"adef0a0d607b9ea2ac60044e03b3c49f48f0469c1ace385ba7fd21a03d4bc517","last_reissued_at":"2026-05-18T02:23:14.980074Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:23:14.980074Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multi-angle effects in self-induced oscillations for different supernova neutrino fluxes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"hep-ph","authors_text":"Alessandro Mirizzi (Hamburg U., II Inst. Theor. Phys.), Ricard Tom\\`as (Hamburg U.","submitted_at":"2010-12-06T21:17:07Z","abstract_excerpt":"The non-isotropic nature of the neutrino emission from a supernova (SN) core might potentially affect the flavor evolution of the neutrino ensemble, via neutrino-neutrino interactions in the deepest SN regions. We investigate the dependence of these \"multi-angle effects\" on the original SN neutrino fluxes in a three-flavor framework. We show that the pattern of the spectral crossings (energies where F_\\nu_e= F_\\nu_x, and F_\\bar\\nu_e= F_\\bar\\nu_x) is crucial in determining the impact of multi-angle effects on the flavor evolution. For neutrino spectra presenting only a single-crossing, synchron"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1012.1339","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":""},"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":"1012.1339","created_at":"2026-05-18T02:23:14.980144+00:00"},{"alias_kind":"arxiv_version","alias_value":"1012.1339v2","created_at":"2026-05-18T02:23:14.980144+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1012.1339","created_at":"2026-05-18T02:23:14.980144+00:00"},{"alias_kind":"pith_short_12","alias_value":"VXXQUDLAPOPK","created_at":"2026-05-18T12:26:15.391820+00:00"},{"alias_kind":"pith_short_16","alias_value":"VXXQUDLAPOPKFLDA","created_at":"2026-05-18T12:26:15.391820+00:00"},{"alias_kind":"pith_short_8","alias_value":"VXXQUDLA","created_at":"2026-05-18T12:26:15.391820+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VXXQUDLAPOPKFLDAARHAHM6ET5","json":"https://pith.science/pith/VXXQUDLAPOPKFLDAARHAHM6ET5.json","graph_json":"https://pith.science/api/pith-number/VXXQUDLAPOPKFLDAARHAHM6ET5/graph.json","events_json":"https://pith.science/api/pith-number/VXXQUDLAPOPKFLDAARHAHM6ET5/events.json","paper":"https://pith.science/paper/VXXQUDLA"},"agent_actions":{"view_html":"https://pith.science/pith/VXXQUDLAPOPKFLDAARHAHM6ET5","download_json":"https://pith.science/pith/VXXQUDLAPOPKFLDAARHAHM6ET5.json","view_paper":"https://pith.science/paper/VXXQUDLA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1012.1339&json=true","fetch_graph":"https://pith.science/api/pith-number/VXXQUDLAPOPKFLDAARHAHM6ET5/graph.json","fetch_events":"https://pith.science/api/pith-number/VXXQUDLAPOPKFLDAARHAHM6ET5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VXXQUDLAPOPKFLDAARHAHM6ET5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VXXQUDLAPOPKFLDAARHAHM6ET5/action/storage_attestation","attest_author":"https://pith.science/pith/VXXQUDLAPOPKFLDAARHAHM6ET5/action/author_attestation","sign_citation":"https://pith.science/pith/VXXQUDLAPOPKFLDAARHAHM6ET5/action/citation_signature","submit_replication":"https://pith.science/pith/VXXQUDLAPOPKFLDAARHAHM6ET5/action/replication_record"}},"created_at":"2026-05-18T02:23:14.980144+00:00","updated_at":"2026-05-18T02:23:14.980144+00:00"}