{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:EUFYFRYWPIFY6QTHKRY2LO5Z6O","short_pith_number":"pith:EUFYFRYW","schema_version":"1.0","canonical_sha256":"250b82c7167a0b8f42675471a5bbb9f399a3884cc7c2f4b5a3ce8330529afca9","source":{"kind":"arxiv","id":"1608.03274","version":1},"attestation_state":"computed","paper":{"title":"The Status of Multi-Dimensional Core-Collapse Supernova Models","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"B. M\\\"uller (Queen's University Belfast, Monash University)","submitted_at":"2016-08-10T20:00:00Z","abstract_excerpt":"Models of core-collapse supernova explosions powered by the neutrino-driven mechanism have matured considerable in recent years. Explosions at the low-mass end of the progenitor spectrum can routinely be simulated in 1D, 2D, and 3D and allow us to study supernova nucleosynthesis based on first-principle models. Results of nucleosynthesis calculations indicate that supernovae of the lowest masses could be important contributors of some lighter n-rich elements beyond iron. The explosion mechanism of more massive stars is still under investigation, although first 3D models of neutrino-driven expl"},"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":"1608.03274","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-08-10T20:00:00Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"3387b45bbc69522b8696898cac8144e05829499170dadce165b533be11e6b309","abstract_canon_sha256":"4b0203da38e2f0c742fcbfe961797a036ada54458c38594c4e1ae192a61de642"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:03:17.612017Z","signature_b64":"zPwcR1WOKxjGieeCAb5nQtV7p0yq7Wp8RMQzZHJhF7q5y/Cg+0bGui/SIChkM+Ues7jVtX6d1QtaWZ26+LEjCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"250b82c7167a0b8f42675471a5bbb9f399a3884cc7c2f4b5a3ce8330529afca9","last_reissued_at":"2026-05-18T01:03:17.611383Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:03:17.611383Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Status of Multi-Dimensional Core-Collapse Supernova Models","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"B. M\\\"uller (Queen's University Belfast, Monash University)","submitted_at":"2016-08-10T20:00:00Z","abstract_excerpt":"Models of core-collapse supernova explosions powered by the neutrino-driven mechanism have matured considerable in recent years. Explosions at the low-mass end of the progenitor spectrum can routinely be simulated in 1D, 2D, and 3D and allow us to study supernova nucleosynthesis based on first-principle models. Results of nucleosynthesis calculations indicate that supernovae of the lowest masses could be important contributors of some lighter n-rich elements beyond iron. The explosion mechanism of more massive stars is still under investigation, although first 3D models of neutrino-driven expl"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.03274","kind":"arxiv","version":1},"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":"1608.03274","created_at":"2026-05-18T01:03:17.611480+00:00"},{"alias_kind":"arxiv_version","alias_value":"1608.03274v1","created_at":"2026-05-18T01:03:17.611480+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1608.03274","created_at":"2026-05-18T01:03:17.611480+00:00"},{"alias_kind":"pith_short_12","alias_value":"EUFYFRYWPIFY","created_at":"2026-05-18T12:30:15.759754+00:00"},{"alias_kind":"pith_short_16","alias_value":"EUFYFRYWPIFY6QTH","created_at":"2026-05-18T12:30:15.759754+00:00"},{"alias_kind":"pith_short_8","alias_value":"EUFYFRYW","created_at":"2026-05-18T12:30:15.759754+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2105.01661","citing_title":"The chemical make-up of the Sun: A 2020 vision","ref_index":205,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EUFYFRYWPIFY6QTHKRY2LO5Z6O","json":"https://pith.science/pith/EUFYFRYWPIFY6QTHKRY2LO5Z6O.json","graph_json":"https://pith.science/api/pith-number/EUFYFRYWPIFY6QTHKRY2LO5Z6O/graph.json","events_json":"https://pith.science/api/pith-number/EUFYFRYWPIFY6QTHKRY2LO5Z6O/events.json","paper":"https://pith.science/paper/EUFYFRYW"},"agent_actions":{"view_html":"https://pith.science/pith/EUFYFRYWPIFY6QTHKRY2LO5Z6O","download_json":"https://pith.science/pith/EUFYFRYWPIFY6QTHKRY2LO5Z6O.json","view_paper":"https://pith.science/paper/EUFYFRYW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1608.03274&json=true","fetch_graph":"https://pith.science/api/pith-number/EUFYFRYWPIFY6QTHKRY2LO5Z6O/graph.json","fetch_events":"https://pith.science/api/pith-number/EUFYFRYWPIFY6QTHKRY2LO5Z6O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EUFYFRYWPIFY6QTHKRY2LO5Z6O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EUFYFRYWPIFY6QTHKRY2LO5Z6O/action/storage_attestation","attest_author":"https://pith.science/pith/EUFYFRYWPIFY6QTHKRY2LO5Z6O/action/author_attestation","sign_citation":"https://pith.science/pith/EUFYFRYWPIFY6QTHKRY2LO5Z6O/action/citation_signature","submit_replication":"https://pith.science/pith/EUFYFRYWPIFY6QTHKRY2LO5Z6O/action/replication_record"}},"created_at":"2026-05-18T01:03:17.611480+00:00","updated_at":"2026-05-18T01:03:17.611480+00:00"}