{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:SBVZI3WSKF6U5PQWWO2WUPNZOV","short_pith_number":"pith:SBVZI3WS","schema_version":"1.0","canonical_sha256":"906b946ed2517d4ebe16b3b56a3db9755e1f20e8792f3c8b27a12d5937e52223","source":{"kind":"arxiv","id":"2011.04769","version":1},"attestation_state":"computed","paper":{"title":"From supernova to supernova remnant: comparison of thermonuclear explosion models","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Donald C. Warren, Florian Lach, Friedrich K. Roepke, Gilles Ferrand, Hiroyoshi Iwasaki, Ivo R. Seitenzahl, Masaomi Ono, Shigehiro Nagataki, Toshiki Sato","submitted_at":"2020-11-09T21:12:57Z","abstract_excerpt":"Progress in the three-dimensional modeling of supernovae (SN) prompts us to revisit the supernova remnant (SNR) phase. We continue our study of the imprint of a thermonuclear explosion on the SNR it produces, that we started with a delayed-detonation model of a Chandrasekhar-mass white dwarf. Here we compare two different types of explosion models, each with two variants: two delayed detonation models (N100ddt, N5ddt) and two pure deflagration models (N100def, N5def), where the N number parametrizes the ignition. The output of each SN simulation is used as input of a SNR simulation carried on "},"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":"2011.04769","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-11-09T21:12:57Z","cross_cats_sorted":[],"title_canon_sha256":"e7f0a713a681967dc2f03b22815c62b2eface23419c3dbe0138d78df67545baa","abstract_canon_sha256":"a252ed3da028763fa70323995b06ff5f9d911e3a59f6863aeb6c5567591e9d00"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:07:51.179625Z","signature_b64":"RU/Bevpecmk7ltYMV5bZuxypbuONIj3bZjaPVWBJDbwXKqggvO+BsBvEchRkn6HNQsv9TBVOLOY/we6esViOCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"906b946ed2517d4ebe16b3b56a3db9755e1f20e8792f3c8b27a12d5937e52223","last_reissued_at":"2026-07-05T02:07:51.179186Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:07:51.179186Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"From supernova to supernova remnant: comparison of thermonuclear explosion models","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Donald C. Warren, Florian Lach, Friedrich K. Roepke, Gilles Ferrand, Hiroyoshi Iwasaki, Ivo R. Seitenzahl, Masaomi Ono, Shigehiro Nagataki, Toshiki Sato","submitted_at":"2020-11-09T21:12:57Z","abstract_excerpt":"Progress in the three-dimensional modeling of supernovae (SN) prompts us to revisit the supernova remnant (SNR) phase. We continue our study of the imprint of a thermonuclear explosion on the SNR it produces, that we started with a delayed-detonation model of a Chandrasekhar-mass white dwarf. Here we compare two different types of explosion models, each with two variants: two delayed detonation models (N100ddt, N5ddt) and two pure deflagration models (N100def, N5def), where the N number parametrizes the ignition. The output of each SN simulation is used as input of a SNR simulation carried on "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2011.04769","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2011.04769/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":"2011.04769","created_at":"2026-07-05T02:07:51.179240+00:00"},{"alias_kind":"arxiv_version","alias_value":"2011.04769v1","created_at":"2026-07-05T02:07:51.179240+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2011.04769","created_at":"2026-07-05T02:07:51.179240+00:00"},{"alias_kind":"pith_short_12","alias_value":"SBVZI3WSKF6U","created_at":"2026-07-05T02:07:51.179240+00:00"},{"alias_kind":"pith_short_16","alias_value":"SBVZI3WSKF6U5PQW","created_at":"2026-07-05T02:07:51.179240+00:00"},{"alias_kind":"pith_short_8","alias_value":"SBVZI3WS","created_at":"2026-07-05T02:07:51.179240+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/SBVZI3WSKF6U5PQWWO2WUPNZOV","json":"https://pith.science/pith/SBVZI3WSKF6U5PQWWO2WUPNZOV.json","graph_json":"https://pith.science/api/pith-number/SBVZI3WSKF6U5PQWWO2WUPNZOV/graph.json","events_json":"https://pith.science/api/pith-number/SBVZI3WSKF6U5PQWWO2WUPNZOV/events.json","paper":"https://pith.science/paper/SBVZI3WS"},"agent_actions":{"view_html":"https://pith.science/pith/SBVZI3WSKF6U5PQWWO2WUPNZOV","download_json":"https://pith.science/pith/SBVZI3WSKF6U5PQWWO2WUPNZOV.json","view_paper":"https://pith.science/paper/SBVZI3WS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2011.04769&json=true","fetch_graph":"https://pith.science/api/pith-number/SBVZI3WSKF6U5PQWWO2WUPNZOV/graph.json","fetch_events":"https://pith.science/api/pith-number/SBVZI3WSKF6U5PQWWO2WUPNZOV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SBVZI3WSKF6U5PQWWO2WUPNZOV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SBVZI3WSKF6U5PQWWO2WUPNZOV/action/storage_attestation","attest_author":"https://pith.science/pith/SBVZI3WSKF6U5PQWWO2WUPNZOV/action/author_attestation","sign_citation":"https://pith.science/pith/SBVZI3WSKF6U5PQWWO2WUPNZOV/action/citation_signature","submit_replication":"https://pith.science/pith/SBVZI3WSKF6U5PQWWO2WUPNZOV/action/replication_record"}},"created_at":"2026-07-05T02:07:51.179240+00:00","updated_at":"2026-07-05T02:07:51.179240+00:00"}