{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2012:CSKIWH7JBDKSMIQVAEQ363ZRKY","short_pith_number":"pith:CSKIWH7J","canonical_record":{"source":{"id":"1203.1484","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2012-03-07T14:34:32Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"5c56dd5aba828dd6fe9ae39cf36526ba6815145e725d0a647fb8514611c2b9cc","abstract_canon_sha256":"56167bd637b16affb3fbabda00f41509e748c14a969b940fc0257e726df4c48a"},"schema_version":"1.0"},"canonical_sha256":"14948b1fe908d52622150121bf6f31560ab1b1436009de234c0219a68233f1a2","source":{"kind":"arxiv","id":"1203.1484","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1203.1484","created_at":"2026-05-18T01:58:13Z"},{"alias_kind":"arxiv_version","alias_value":"1203.1484v2","created_at":"2026-05-18T01:58:13Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1203.1484","created_at":"2026-05-18T01:58:13Z"},{"alias_kind":"pith_short_12","alias_value":"CSKIWH7JBDKS","created_at":"2026-05-18T12:27:01Z"},{"alias_kind":"pith_short_16","alias_value":"CSKIWH7JBDKSMIQV","created_at":"2026-05-18T12:27:01Z"},{"alias_kind":"pith_short_8","alias_value":"CSKIWH7J","created_at":"2026-05-18T12:27:01Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2012:CSKIWH7JBDKSMIQVAEQ363ZRKY","target":"record","payload":{"canonical_record":{"source":{"id":"1203.1484","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2012-03-07T14:34:32Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"5c56dd5aba828dd6fe9ae39cf36526ba6815145e725d0a647fb8514611c2b9cc","abstract_canon_sha256":"56167bd637b16affb3fbabda00f41509e748c14a969b940fc0257e726df4c48a"},"schema_version":"1.0"},"canonical_sha256":"14948b1fe908d52622150121bf6f31560ab1b1436009de234c0219a68233f1a2","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:13.731253Z","signature_b64":"Xkrow3UAs1fPAP9aOZc9Mt80e3QqAGYLRsHLGV4K2ff8qNfL68rdMTHNkKkdq7Q4emTk9Pr/95/HUE5iLLsVCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"14948b1fe908d52622150121bf6f31560ab1b1436009de234c0219a68233f1a2","last_reissued_at":"2026-05-18T01:58:13.730798Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:13.730798Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1203.1484","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:58:13Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"P21MKts8yrRon9My+QasNgG/CnRptNyFBwnousTYjBAsMysOkqV+r7Kp3vXPfvoAzrsMXgezNb8jSjS9azU4Dw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-30T12:34:46.435337Z"},"content_sha256":"109206adc08319c3c7aa74de1b66c8a19335f8f4b72f49ccda5522eb16985d7d","schema_version":"1.0","event_id":"sha256:109206adc08319c3c7aa74de1b66c8a19335f8f4b72f49ccda5522eb16985d7d"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2012:CSKIWH7JBDKSMIQVAEQ363ZRKY","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Stability analysis of collective neutrino oscillations in the supernova accretion phase with realistic energy and angle distributions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Alessandro Mirizzi (Hamburg U., II Inst. Theor. Phys.), Ninetta Saviano (Hamburg U., Sovan Chakraborty (Hamburg U., Technische Univ. Darmstadt), Tobias Fischer (GSI","submitted_at":"2012-03-07T14:34:32Z","abstract_excerpt":"We revisit our previous results on the matter suppression of self-induced neutrino flavor conversions during a supernova (SN) accretion phase, performing a linearized stability analysis of the neutrino equations of motion, in the presence of realistic SN density profiles. In our previous numerical study, we used a simplified model based on an isotropic neutrino emission with a single typical energy. Here, we take into account realistic neutrino energy and angle distributions. We find that multi-energy effects have a sub-leading impact in the flavor stability of the SN neutrino fluxes with resp"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1203.1484","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:58:13Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"inuF07CeTW+cua8XhV6LWgE1pHGy4B6/WWE6GuKIfboDU8PBfmtzzZ907TgGBDzcfB7rdkMfN0m220hP/oq8AQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-30T12:34:46.435883Z"},"content_sha256":"7a23b06bd5f6856af15041ad3a84490282c8acd328dd91f024c283515e4d3887","schema_version":"1.0","event_id":"sha256:7a23b06bd5f6856af15041ad3a84490282c8acd328dd91f024c283515e4d3887"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/CSKIWH7JBDKSMIQVAEQ363ZRKY/bundle.json","state_url":"https://pith.science/pith/CSKIWH7JBDKSMIQVAEQ363ZRKY/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/CSKIWH7JBDKSMIQVAEQ363ZRKY/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-30T12:34:46Z","links":{"resolver":"https://pith.science/pith/CSKIWH7JBDKSMIQVAEQ363ZRKY","bundle":"https://pith.science/pith/CSKIWH7JBDKSMIQVAEQ363ZRKY/bundle.json","state":"https://pith.science/pith/CSKIWH7JBDKSMIQVAEQ363ZRKY/state.json","well_known_bundle":"https://pith.science/.well-known/pith/CSKIWH7JBDKSMIQVAEQ363ZRKY/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2012:CSKIWH7JBDKSMIQVAEQ363ZRKY","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"56167bd637b16affb3fbabda00f41509e748c14a969b940fc0257e726df4c48a","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2012-03-07T14:34:32Z","title_canon_sha256":"5c56dd5aba828dd6fe9ae39cf36526ba6815145e725d0a647fb8514611c2b9cc"},"schema_version":"1.0","source":{"id":"1203.1484","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1203.1484","created_at":"2026-05-18T01:58:13Z"},{"alias_kind":"arxiv_version","alias_value":"1203.1484v2","created_at":"2026-05-18T01:58:13Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1203.1484","created_at":"2026-05-18T01:58:13Z"},{"alias_kind":"pith_short_12","alias_value":"CSKIWH7JBDKS","created_at":"2026-05-18T12:27:01Z"},{"alias_kind":"pith_short_16","alias_value":"CSKIWH7JBDKSMIQV","created_at":"2026-05-18T12:27:01Z"},{"alias_kind":"pith_short_8","alias_value":"CSKIWH7J","created_at":"2026-05-18T12:27:01Z"}],"graph_snapshots":[{"event_id":"sha256:7a23b06bd5f6856af15041ad3a84490282c8acd328dd91f024c283515e4d3887","target":"graph","created_at":"2026-05-18T01:58:13Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We revisit our previous results on the matter suppression of self-induced neutrino flavor conversions during a supernova (SN) accretion phase, performing a linearized stability analysis of the neutrino equations of motion, in the presence of realistic SN density profiles. In our previous numerical study, we used a simplified model based on an isotropic neutrino emission with a single typical energy. Here, we take into account realistic neutrino energy and angle distributions. We find that multi-energy effects have a sub-leading impact in the flavor stability of the SN neutrino fluxes with resp","authors_text":"Alessandro Mirizzi (Hamburg U., II Inst. Theor. Phys.), Ninetta Saviano (Hamburg U., Sovan Chakraborty (Hamburg U., Technische Univ. Darmstadt), Tobias Fischer (GSI","cross_cats":["astro-ph.HE"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2012-03-07T14:34:32Z","title":"Stability analysis of collective neutrino oscillations in the supernova accretion phase with realistic energy and angle distributions"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1203.1484","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:109206adc08319c3c7aa74de1b66c8a19335f8f4b72f49ccda5522eb16985d7d","target":"record","created_at":"2026-05-18T01:58:13Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"56167bd637b16affb3fbabda00f41509e748c14a969b940fc0257e726df4c48a","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2012-03-07T14:34:32Z","title_canon_sha256":"5c56dd5aba828dd6fe9ae39cf36526ba6815145e725d0a647fb8514611c2b9cc"},"schema_version":"1.0","source":{"id":"1203.1484","kind":"arxiv","version":2}},"canonical_sha256":"14948b1fe908d52622150121bf6f31560ab1b1436009de234c0219a68233f1a2","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"14948b1fe908d52622150121bf6f31560ab1b1436009de234c0219a68233f1a2","first_computed_at":"2026-05-18T01:58:13.730798Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:58:13.730798Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"Xkrow3UAs1fPAP9aOZc9Mt80e3QqAGYLRsHLGV4K2ff8qNfL68rdMTHNkKkdq7Q4emTk9Pr/95/HUE5iLLsVCQ==","signature_status":"signed_v1","signed_at":"2026-05-18T01:58:13.731253Z","signed_message":"canonical_sha256_bytes"},"source_id":"1203.1484","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:109206adc08319c3c7aa74de1b66c8a19335f8f4b72f49ccda5522eb16985d7d","sha256:7a23b06bd5f6856af15041ad3a84490282c8acd328dd91f024c283515e4d3887"],"state_sha256":"7bb55ef616c1b44512cd1afaa997bceab2cf66a4cb3523e9aa21718b1972c86f"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"2QCdDTWpPSENR+O5oiL/jHeMFsLYb2QmTrtWZmduZ10EkcN+Y//L5BN0eCt0dM+m2mpHdiXP0HUILJgiyFxuDQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-30T12:34:46.439138Z","bundle_sha256":"d9346b36e0b3a087f6a71abaa3893dbafde485982a07cd4b6b8af81464a67d8c"}}