{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:ZFWZQASK3HFQTA3E2MT6HYJA7M","short_pith_number":"pith:ZFWZQASK","schema_version":"1.0","canonical_sha256":"c96d98024ad9cb098364d327e3e120fb084ff59312270ec013f2f194e0956812","source":{"kind":"arxiv","id":"1706.05438","version":2},"attestation_state":"computed","paper":{"title":"Numerical Simulation of the Hydrodynamical Combustion to Strange Quark Matter in the Trapped Neutrino Regime","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"nucl-th","authors_text":"Amir Ouyed, Prashanth Jaikumar, Rachid Ouyed","submitted_at":"2017-06-16T21:52:06Z","abstract_excerpt":"We simulate and study the microphysics of combustion (flame burning) of two flavored quark matter (u, d) to three flavoured quark matter (u,d,s) in a trapped neutrino regime applicable to conditions prevailing in a hot proto-neutron star. The reaction-diffusion-advection equations for (u,d) to (u,d,s) combustion are coupled with neutrino transport, which is modelled through a flux-limited diffusion scheme. The flame speed is proportional to initial lepton fraction because of the release of electron chemical potential as heat, and reaches a steady-state burning speed of (0.001-0.008)c. We find "},"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":"1706.05438","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2017-06-16T21:52:06Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"b3413b23d64ab9b00a3d7c155bfef95c355f386d5ded31716bda44f20b6dd2da","abstract_canon_sha256":"84fa941f4cddc84798ddcdf4494892f17e71e9e22e9be318547ab8f4bdda92ea"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:25:57.188576Z","signature_b64":"ixmXKx/y57vqV6vdb77tK3c0YrsjKbjm7QHh5VMKVoAp4ylGNqVH+JfoGx995ak5+XyOe4H7qz5l5Nw+dAk6Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c96d98024ad9cb098364d327e3e120fb084ff59312270ec013f2f194e0956812","last_reissued_at":"2026-05-18T00:25:57.187962Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:25:57.187962Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Numerical Simulation of the Hydrodynamical Combustion to Strange Quark Matter in the Trapped Neutrino Regime","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"nucl-th","authors_text":"Amir Ouyed, Prashanth Jaikumar, Rachid Ouyed","submitted_at":"2017-06-16T21:52:06Z","abstract_excerpt":"We simulate and study the microphysics of combustion (flame burning) of two flavored quark matter (u, d) to three flavoured quark matter (u,d,s) in a trapped neutrino regime applicable to conditions prevailing in a hot proto-neutron star. The reaction-diffusion-advection equations for (u,d) to (u,d,s) combustion are coupled with neutrino transport, which is modelled through a flux-limited diffusion scheme. The flame speed is proportional to initial lepton fraction because of the release of electron chemical potential as heat, and reaches a steady-state burning speed of (0.001-0.008)c. We find "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.05438","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":"1706.05438","created_at":"2026-05-18T00:25:57.188047+00:00"},{"alias_kind":"arxiv_version","alias_value":"1706.05438v2","created_at":"2026-05-18T00:25:57.188047+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.05438","created_at":"2026-05-18T00:25:57.188047+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZFWZQASK3HFQ","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZFWZQASK3HFQTA3E","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZFWZQASK","created_at":"2026-05-18T12:31:59.375834+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/ZFWZQASK3HFQTA3E2MT6HYJA7M","json":"https://pith.science/pith/ZFWZQASK3HFQTA3E2MT6HYJA7M.json","graph_json":"https://pith.science/api/pith-number/ZFWZQASK3HFQTA3E2MT6HYJA7M/graph.json","events_json":"https://pith.science/api/pith-number/ZFWZQASK3HFQTA3E2MT6HYJA7M/events.json","paper":"https://pith.science/paper/ZFWZQASK"},"agent_actions":{"view_html":"https://pith.science/pith/ZFWZQASK3HFQTA3E2MT6HYJA7M","download_json":"https://pith.science/pith/ZFWZQASK3HFQTA3E2MT6HYJA7M.json","view_paper":"https://pith.science/paper/ZFWZQASK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1706.05438&json=true","fetch_graph":"https://pith.science/api/pith-number/ZFWZQASK3HFQTA3E2MT6HYJA7M/graph.json","fetch_events":"https://pith.science/api/pith-number/ZFWZQASK3HFQTA3E2MT6HYJA7M/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZFWZQASK3HFQTA3E2MT6HYJA7M/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZFWZQASK3HFQTA3E2MT6HYJA7M/action/storage_attestation","attest_author":"https://pith.science/pith/ZFWZQASK3HFQTA3E2MT6HYJA7M/action/author_attestation","sign_citation":"https://pith.science/pith/ZFWZQASK3HFQTA3E2MT6HYJA7M/action/citation_signature","submit_replication":"https://pith.science/pith/ZFWZQASK3HFQTA3E2MT6HYJA7M/action/replication_record"}},"created_at":"2026-05-18T00:25:57.188047+00:00","updated_at":"2026-05-18T00:25:57.188047+00:00"}