{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:RSZBE7KMA2DKBF6SKGXTYY6LRL","short_pith_number":"pith:RSZBE7KM","schema_version":"1.0","canonical_sha256":"8cb2127d4c0686a097d251af3c63cb8afeb0571898b6c43b30ea87b6e040b914","source":{"kind":"arxiv","id":"1204.0512","version":2},"attestation_state":"computed","paper":{"title":"Correlated Gravitational Wave and Neutrino Signals from General-Relativistic Rapidly Rotating Iron Core Collapse","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"1), (2) Cal Poly San Luis Obispo, (3) Princeton, (4) Perimeter Institute), A. Burrows (3), C. D. Ott (1), C. Reisswig (1), E. Abdikamalov (1), E. O'Connor (1), E. Schnetter (4) ((1) Caltech, P. Kalmus (1), R. Haas (1), S. Drasco (2","submitted_at":"2012-04-02T20:00:00Z","abstract_excerpt":"We present results from a new set of 3D general-relativistic hydrodynamic simulations of rotating iron core collapse. We assume octant symmetry and focus on axisymmetric collapse, bounce, the early postbounce evolution, and the associated gravitational wave (GW) and neutrino signals. We employ a finite-temperature nuclear equation of state, parameterized electron capture in the collapse phase, and a multi-species neutrino leakage scheme after bounce. The latter captures the important effects of deleptonization, neutrino cooling and heating and enables approximate predictions for the neutrino l"},"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":"1204.0512","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-04-02T20:00:00Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"aadbc68f2be99b0814805273f9ab70d153573cde4696c8508ebfd6bdab0816cb","abstract_canon_sha256":"3638a6b60cc4793f07b7ad423f80d0865526716370b9cb9714515f2d9fbc7d67"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:22:42.520367Z","signature_b64":"rX87jjxe9GDpAFjI7jJeyEQAdwcF7unAI4+PMSMnuwWDS/s0857L9s+Be3+XMGDjfwTKo7G7jhUo7P5/J4aWBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8cb2127d4c0686a097d251af3c63cb8afeb0571898b6c43b30ea87b6e040b914","last_reissued_at":"2026-05-18T03:22:42.519664Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:22:42.519664Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Correlated Gravitational Wave and Neutrino Signals from General-Relativistic Rapidly Rotating Iron Core Collapse","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"1), (2) Cal Poly San Luis Obispo, (3) Princeton, (4) Perimeter Institute), A. Burrows (3), C. D. Ott (1), C. Reisswig (1), E. Abdikamalov (1), E. O'Connor (1), E. Schnetter (4) ((1) Caltech, P. Kalmus (1), R. Haas (1), S. Drasco (2","submitted_at":"2012-04-02T20:00:00Z","abstract_excerpt":"We present results from a new set of 3D general-relativistic hydrodynamic simulations of rotating iron core collapse. We assume octant symmetry and focus on axisymmetric collapse, bounce, the early postbounce evolution, and the associated gravitational wave (GW) and neutrino signals. We employ a finite-temperature nuclear equation of state, parameterized electron capture in the collapse phase, and a multi-species neutrino leakage scheme after bounce. The latter captures the important effects of deleptonization, neutrino cooling and heating and enables approximate predictions for the neutrino l"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1204.0512","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1204.0512","created_at":"2026-05-18T03:22:42.519756+00:00"},{"alias_kind":"arxiv_version","alias_value":"1204.0512v2","created_at":"2026-05-18T03:22:42.519756+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1204.0512","created_at":"2026-05-18T03:22:42.519756+00:00"},{"alias_kind":"pith_short_12","alias_value":"RSZBE7KMA2DK","created_at":"2026-05-18T12:27:20.899486+00:00"},{"alias_kind":"pith_short_16","alias_value":"RSZBE7KMA2DKBF6S","created_at":"2026-05-18T12:27:20.899486+00:00"},{"alias_kind":"pith_short_8","alias_value":"RSZBE7KM","created_at":"2026-05-18T12:27:20.899486+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.04896","citing_title":"Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors","ref_index":47,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RSZBE7KMA2DKBF6SKGXTYY6LRL","json":"https://pith.science/pith/RSZBE7KMA2DKBF6SKGXTYY6LRL.json","graph_json":"https://pith.science/api/pith-number/RSZBE7KMA2DKBF6SKGXTYY6LRL/graph.json","events_json":"https://pith.science/api/pith-number/RSZBE7KMA2DKBF6SKGXTYY6LRL/events.json","paper":"https://pith.science/paper/RSZBE7KM"},"agent_actions":{"view_html":"https://pith.science/pith/RSZBE7KMA2DKBF6SKGXTYY6LRL","download_json":"https://pith.science/pith/RSZBE7KMA2DKBF6SKGXTYY6LRL.json","view_paper":"https://pith.science/paper/RSZBE7KM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1204.0512&json=true","fetch_graph":"https://pith.science/api/pith-number/RSZBE7KMA2DKBF6SKGXTYY6LRL/graph.json","fetch_events":"https://pith.science/api/pith-number/RSZBE7KMA2DKBF6SKGXTYY6LRL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RSZBE7KMA2DKBF6SKGXTYY6LRL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RSZBE7KMA2DKBF6SKGXTYY6LRL/action/storage_attestation","attest_author":"https://pith.science/pith/RSZBE7KMA2DKBF6SKGXTYY6LRL/action/author_attestation","sign_citation":"https://pith.science/pith/RSZBE7KMA2DKBF6SKGXTYY6LRL/action/citation_signature","submit_replication":"https://pith.science/pith/RSZBE7KMA2DKBF6SKGXTYY6LRL/action/replication_record"}},"created_at":"2026-05-18T03:22:42.519756+00:00","updated_at":"2026-05-18T03:22:42.519756+00:00"}