{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:GG2JOUMWXJ2UZB4XTXBRH3PBSX","short_pith_number":"pith:GG2JOUMW","schema_version":"1.0","canonical_sha256":"31b4975196ba754c87979dc313ede195c60b71f9e3bddf21cadd1e148fbc427f","source":{"kind":"arxiv","id":"1303.5055","version":1},"attestation_state":"computed","paper":{"title":"Very Low Energy Supernovae from Neutrino Mass Loss","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Elizabeth Lovegrove, Stan Woosley","submitted_at":"2013-03-20T20:00:04Z","abstract_excerpt":"The continuing difficulty of achieving a reliable explosion in simulations of core-collapse supernovae, especially for more massive stars, has led to speculation concerning the observable transients that might be produced if such a supernova fails. Even if a prompt outgoing shock fails to form in a collapsing presupernova star, one must still consider the hydrodynamic response of the star to the abrupt loss of mass via neutrinos as the core forms a protoneutron star. Following a suggestion by Nadezhin (1980), we calculate the hydrodynamical responses of typical supernova progenitor stars to th"},"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":"1303.5055","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-03-20T20:00:04Z","cross_cats_sorted":[],"title_canon_sha256":"ee828244991a626de4f94b5dc43ef38634d02bb4d5d7beb8c9534deae6780285","abstract_canon_sha256":"81f7b8aca6538e8a452b01ad317c5d1ac9fbfba3affca42b4a9e95992487b128"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:25:24.835938Z","signature_b64":"cf7oB11XwnJFZOsuQnV+odwXI+HvI0LTubDk+vtgUuiGKrZB5/sE2C2XiUKUzyT7sjgbpzaFq8rtKGTSO6AOCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"31b4975196ba754c87979dc313ede195c60b71f9e3bddf21cadd1e148fbc427f","last_reissued_at":"2026-05-18T03:25:24.835075Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:25:24.835075Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Very Low Energy Supernovae from Neutrino Mass Loss","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Elizabeth Lovegrove, Stan Woosley","submitted_at":"2013-03-20T20:00:04Z","abstract_excerpt":"The continuing difficulty of achieving a reliable explosion in simulations of core-collapse supernovae, especially for more massive stars, has led to speculation concerning the observable transients that might be produced if such a supernova fails. Even if a prompt outgoing shock fails to form in a collapsing presupernova star, one must still consider the hydrodynamic response of the star to the abrupt loss of mass via neutrinos as the core forms a protoneutron star. Following a suggestion by Nadezhin (1980), we calculate the hydrodynamical responses of typical supernova progenitor stars to th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.5055","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":"1303.5055","created_at":"2026-05-18T03:25:24.835209+00:00"},{"alias_kind":"arxiv_version","alias_value":"1303.5055v1","created_at":"2026-05-18T03:25:24.835209+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1303.5055","created_at":"2026-05-18T03:25:24.835209+00:00"},{"alias_kind":"pith_short_12","alias_value":"GG2JOUMWXJ2U","created_at":"2026-05-18T12:27:45.050594+00:00"},{"alias_kind":"pith_short_16","alias_value":"GG2JOUMWXJ2UZB4X","created_at":"2026-05-18T12:27:45.050594+00:00"},{"alias_kind":"pith_short_8","alias_value":"GG2JOUMW","created_at":"2026-05-18T12:27:45.050594+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/GG2JOUMWXJ2UZB4XTXBRH3PBSX","json":"https://pith.science/pith/GG2JOUMWXJ2UZB4XTXBRH3PBSX.json","graph_json":"https://pith.science/api/pith-number/GG2JOUMWXJ2UZB4XTXBRH3PBSX/graph.json","events_json":"https://pith.science/api/pith-number/GG2JOUMWXJ2UZB4XTXBRH3PBSX/events.json","paper":"https://pith.science/paper/GG2JOUMW"},"agent_actions":{"view_html":"https://pith.science/pith/GG2JOUMWXJ2UZB4XTXBRH3PBSX","download_json":"https://pith.science/pith/GG2JOUMWXJ2UZB4XTXBRH3PBSX.json","view_paper":"https://pith.science/paper/GG2JOUMW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1303.5055&json=true","fetch_graph":"https://pith.science/api/pith-number/GG2JOUMWXJ2UZB4XTXBRH3PBSX/graph.json","fetch_events":"https://pith.science/api/pith-number/GG2JOUMWXJ2UZB4XTXBRH3PBSX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GG2JOUMWXJ2UZB4XTXBRH3PBSX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GG2JOUMWXJ2UZB4XTXBRH3PBSX/action/storage_attestation","attest_author":"https://pith.science/pith/GG2JOUMWXJ2UZB4XTXBRH3PBSX/action/author_attestation","sign_citation":"https://pith.science/pith/GG2JOUMWXJ2UZB4XTXBRH3PBSX/action/citation_signature","submit_replication":"https://pith.science/pith/GG2JOUMWXJ2UZB4XTXBRH3PBSX/action/replication_record"}},"created_at":"2026-05-18T03:25:24.835209+00:00","updated_at":"2026-05-18T03:25:24.835209+00:00"}