{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:GKPDTP3KBRKNAWA6BNS2GFQC6G","short_pith_number":"pith:GKPDTP3K","schema_version":"1.0","canonical_sha256":"329e39bf6a0c54d0581e0b65a31602f1b8ecf00f0b7c927fce3da9492afbeb39","source":{"kind":"arxiv","id":"2311.00033","version":2},"attestation_state":"computed","paper":{"title":"Comprehensive constraints on heavy sterile neutrinos from core-collapse supernovae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Alessandro Mirizzi, Giuseppe Lucente, Leonardo Mastrototaro, Pasquale Dario Serpico, Pierluca Carenza","submitted_at":"2023-10-31T18:00:02Z","abstract_excerpt":"Sterile neutrinos with masses up to $\\mathcal{O} (100)$ MeV can be copiously produced in a supernova (SN) core, through the mixing with active neutrinos. In this regard the SN 1987A detection of neutrino events has been used to put constraints on active-sterile neutrino mixing, exploiting the well-known SN cooling argument. We refine the calculation of this limit including neutral current interactions with nucleons, that constitute the dominant channel for sterile neutrino production. We also include, for the first time, the charged current interactions between sterile neutrinos and muons, rel"},"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":"2311.00033","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2023-10-31T18:00:02Z","cross_cats_sorted":[],"title_canon_sha256":"20203bad8622a24793c3de442979380460a67302a1d7db9189eb508a018a4f8a","abstract_canon_sha256":"df59d786c7ebe7f45708d379fdbde4562afc49462ccafa74978c324024f8deb3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:54:05.639952Z","signature_b64":"7fXPS4oOLQOoMx7omLiwTmKyD30XyCoSo1lx7zU/bGd0E/CFbhnltsFWLAJV7zGgj/nYTP6YuJ3NfBn4YE7XDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"329e39bf6a0c54d0581e0b65a31602f1b8ecf00f0b7c927fce3da9492afbeb39","last_reissued_at":"2026-07-05T07:54:05.639405Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:54:05.639405Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Comprehensive constraints on heavy sterile neutrinos from core-collapse supernovae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Alessandro Mirizzi, Giuseppe Lucente, Leonardo Mastrototaro, Pasquale Dario Serpico, Pierluca Carenza","submitted_at":"2023-10-31T18:00:02Z","abstract_excerpt":"Sterile neutrinos with masses up to $\\mathcal{O} (100)$ MeV can be copiously produced in a supernova (SN) core, through the mixing with active neutrinos. In this regard the SN 1987A detection of neutrino events has been used to put constraints on active-sterile neutrino mixing, exploiting the well-known SN cooling argument. We refine the calculation of this limit including neutral current interactions with nucleons, that constitute the dominant channel for sterile neutrino production. We also include, for the first time, the charged current interactions between sterile neutrinos and muons, rel"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.00033","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/2311.00033/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":"2311.00033","created_at":"2026-07-05T07:54:05.639459+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.00033v2","created_at":"2026-07-05T07:54:05.639459+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.00033","created_at":"2026-07-05T07:54:05.639459+00:00"},{"alias_kind":"pith_short_12","alias_value":"GKPDTP3KBRKN","created_at":"2026-07-05T07:54:05.639459+00:00"},{"alias_kind":"pith_short_16","alias_value":"GKPDTP3KBRKNAWA6","created_at":"2026-07-05T07:54:05.639459+00:00"},{"alias_kind":"pith_short_8","alias_value":"GKPDTP3K","created_at":"2026-07-05T07:54:05.639459+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.23769","citing_title":"SN1987A Constraints of Light $\\boldsymbol{Z'}$ with Non-Mixing Polarisations","ref_index":21,"is_internal_anchor":false},{"citing_arxiv_id":"2503.15630","citing_title":"Supernova production of axion-like particles coupling to electrons, reloaded","ref_index":26,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14282","citing_title":"Probing Neutrino Compositeness with Invisible and Displaced Signals","ref_index":63,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GKPDTP3KBRKNAWA6BNS2GFQC6G","json":"https://pith.science/pith/GKPDTP3KBRKNAWA6BNS2GFQC6G.json","graph_json":"https://pith.science/api/pith-number/GKPDTP3KBRKNAWA6BNS2GFQC6G/graph.json","events_json":"https://pith.science/api/pith-number/GKPDTP3KBRKNAWA6BNS2GFQC6G/events.json","paper":"https://pith.science/paper/GKPDTP3K"},"agent_actions":{"view_html":"https://pith.science/pith/GKPDTP3KBRKNAWA6BNS2GFQC6G","download_json":"https://pith.science/pith/GKPDTP3KBRKNAWA6BNS2GFQC6G.json","view_paper":"https://pith.science/paper/GKPDTP3K","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.00033&json=true","fetch_graph":"https://pith.science/api/pith-number/GKPDTP3KBRKNAWA6BNS2GFQC6G/graph.json","fetch_events":"https://pith.science/api/pith-number/GKPDTP3KBRKNAWA6BNS2GFQC6G/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GKPDTP3KBRKNAWA6BNS2GFQC6G/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GKPDTP3KBRKNAWA6BNS2GFQC6G/action/storage_attestation","attest_author":"https://pith.science/pith/GKPDTP3KBRKNAWA6BNS2GFQC6G/action/author_attestation","sign_citation":"https://pith.science/pith/GKPDTP3KBRKNAWA6BNS2GFQC6G/action/citation_signature","submit_replication":"https://pith.science/pith/GKPDTP3KBRKNAWA6BNS2GFQC6G/action/replication_record"}},"created_at":"2026-07-05T07:54:05.639459+00:00","updated_at":"2026-07-05T07:54:05.639459+00:00"}