{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:FUATHJKTYBLBQC3N2WY6N2OZNI","short_pith_number":"pith:FUATHJKT","schema_version":"1.0","canonical_sha256":"2d0133a553c056180b6dd5b1e6e9d96a399ef1546aba22087e830b47263ce7b2","source":{"kind":"arxiv","id":"2007.07926","version":2},"attestation_state":"computed","paper":{"title":"Dispelling a myth on dense neutrino media: fast pairwise conversions depend on energy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Irene Tamborra, Shashank Shalgar","submitted_at":"2020-07-15T18:11:39Z","abstract_excerpt":"Pairwise conversions of neutrinos have complicated the challenging goal of quantifying the relevance of neutrino microphysics in compact astrophysical objects, limiting the ability to perform numerical simulations and encouraging the employment of semi-analytical tools, such as the linear stability analysis. Given the high neutrino density, the dependence of pairwise conversions on the neutrino energy has been deemed to play a negligible role. We show that fast pairwise conversions are affected by the neutrino energy, especially in the non-linear regime. An earlier onset of flavor conversions "},"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":"2007.07926","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-07-15T18:11:39Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"123e5bfcc50716191f6ebdb25cadf78753827e2a23465a4741644f1576b2ec18","abstract_canon_sha256":"3bc171e76698b89be6b59da961bd06b975ef7b5a833894f51d340989e30f1800"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:05:41.900134Z","signature_b64":"9Bp2oFYvkFnJSrFlPwbnTWjMpNSrcdO4JDWyGbK5BdirQe+FjfoG3vukuZ8eXRb04w+9og1PxV0RcOsrdxWcAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2d0133a553c056180b6dd5b1e6e9d96a399ef1546aba22087e830b47263ce7b2","last_reissued_at":"2026-07-05T02:05:41.899722Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:05:41.899722Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dispelling a myth on dense neutrino media: fast pairwise conversions depend on energy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Irene Tamborra, Shashank Shalgar","submitted_at":"2020-07-15T18:11:39Z","abstract_excerpt":"Pairwise conversions of neutrinos have complicated the challenging goal of quantifying the relevance of neutrino microphysics in compact astrophysical objects, limiting the ability to perform numerical simulations and encouraging the employment of semi-analytical tools, such as the linear stability analysis. Given the high neutrino density, the dependence of pairwise conversions on the neutrino energy has been deemed to play a negligible role. We show that fast pairwise conversions are affected by the neutrino energy, especially in the non-linear regime. An earlier onset of flavor conversions "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2007.07926","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/2007.07926/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":"2007.07926","created_at":"2026-07-05T02:05:41.899784+00:00"},{"alias_kind":"arxiv_version","alias_value":"2007.07926v2","created_at":"2026-07-05T02:05:41.899784+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2007.07926","created_at":"2026-07-05T02:05:41.899784+00:00"},{"alias_kind":"pith_short_12","alias_value":"FUATHJKTYBLB","created_at":"2026-07-05T02:05:41.899784+00:00"},{"alias_kind":"pith_short_16","alias_value":"FUATHJKTYBLBQC3N","created_at":"2026-07-05T02:05:41.899784+00:00"},{"alias_kind":"pith_short_8","alias_value":"FUATHJKT","created_at":"2026-07-05T02:05:41.899784+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2412.12268","citing_title":"Pauli blocking: probing beyond-mean-field effects in neutrino flavor evolution","ref_index":49,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FUATHJKTYBLBQC3N2WY6N2OZNI","json":"https://pith.science/pith/FUATHJKTYBLBQC3N2WY6N2OZNI.json","graph_json":"https://pith.science/api/pith-number/FUATHJKTYBLBQC3N2WY6N2OZNI/graph.json","events_json":"https://pith.science/api/pith-number/FUATHJKTYBLBQC3N2WY6N2OZNI/events.json","paper":"https://pith.science/paper/FUATHJKT"},"agent_actions":{"view_html":"https://pith.science/pith/FUATHJKTYBLBQC3N2WY6N2OZNI","download_json":"https://pith.science/pith/FUATHJKTYBLBQC3N2WY6N2OZNI.json","view_paper":"https://pith.science/paper/FUATHJKT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2007.07926&json=true","fetch_graph":"https://pith.science/api/pith-number/FUATHJKTYBLBQC3N2WY6N2OZNI/graph.json","fetch_events":"https://pith.science/api/pith-number/FUATHJKTYBLBQC3N2WY6N2OZNI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FUATHJKTYBLBQC3N2WY6N2OZNI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FUATHJKTYBLBQC3N2WY6N2OZNI/action/storage_attestation","attest_author":"https://pith.science/pith/FUATHJKTYBLBQC3N2WY6N2OZNI/action/author_attestation","sign_citation":"https://pith.science/pith/FUATHJKTYBLBQC3N2WY6N2OZNI/action/citation_signature","submit_replication":"https://pith.science/pith/FUATHJKTYBLBQC3N2WY6N2OZNI/action/replication_record"}},"created_at":"2026-07-05T02:05:41.899784+00:00","updated_at":"2026-07-05T02:05:41.899784+00:00"}