{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2003:5ADJJPSDGAIFXBATRWSDHYXKZQ","short_pith_number":"pith:5ADJJPSD","schema_version":"1.0","canonical_sha256":"e80694be4330105b84138da433e2eacc1900b188f11c965f51584caadd18ba11","source":{"kind":"arxiv","id":"gr-qc/0310030","version":1},"attestation_state":"computed","paper":{"title":"Merger of binary neutron stars of unequal mass in full general relativity","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"gr-qc","authors_text":"Keisuke Taniguchi, Koji Uryu, Masaru Shibata","submitted_at":"2003-10-06T05:10:33Z","abstract_excerpt":"We present results of three dimensional numerical simulations of the merger of unequal-mass binary neutron stars in full general relativity. A $\\Gamma$-law equation of state $P=(\\Gamma-1)\\rho\\epsilon$ is adopted, where $P$, $\\rho$, $\\varep$, and $\\Gamma$ are the pressure, rest mass density, specific internal energy, and the adiabatic constant, respectively. We take $\\Gamma=2$ and the baryon rest-mass ratio $Q_M$ to be in the range 0.85--1. The typical grid size is $(633,633,317)$ for $(x,y,z)$ . We improve several implementations since the latest work. In the present code, the radiation reacti"},"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":"gr-qc/0310030","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"2003-10-06T05:10:33Z","cross_cats_sorted":["astro-ph"],"title_canon_sha256":"cf523c38c666554710a07f3b4ef76cec936d3d5601d4722354c752dac010744b","abstract_canon_sha256":"8526534523db0a7d9a953cca26b1d1ca9b3e039aafe49bf71983e5c4cc175235"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:06:47.367364Z","signature_b64":"OfSmekwTzIqEYh5DFv2uVfn5PYuuK0NfBW+P7OmO8mgtFT01yDANZHDCgoZbiuGzNvQt/BULlok7tTd2iuEUAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e80694be4330105b84138da433e2eacc1900b188f11c965f51584caadd18ba11","last_reissued_at":"2026-05-18T01:06:47.366709Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:06:47.366709Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Merger of binary neutron stars of unequal mass in full general relativity","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"gr-qc","authors_text":"Keisuke Taniguchi, Koji Uryu, Masaru Shibata","submitted_at":"2003-10-06T05:10:33Z","abstract_excerpt":"We present results of three dimensional numerical simulations of the merger of unequal-mass binary neutron stars in full general relativity. A $\\Gamma$-law equation of state $P=(\\Gamma-1)\\rho\\epsilon$ is adopted, where $P$, $\\rho$, $\\varep$, and $\\Gamma$ are the pressure, rest mass density, specific internal energy, and the adiabatic constant, respectively. We take $\\Gamma=2$ and the baryon rest-mass ratio $Q_M$ to be in the range 0.85--1. The typical grid size is $(633,633,317)$ for $(x,y,z)$ . We improve several implementations since the latest work. In the present code, the radiation reacti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/0310030","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":"gr-qc/0310030","created_at":"2026-05-18T01:06:47.366819+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/0310030v1","created_at":"2026-05-18T01:06:47.366819+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/0310030","created_at":"2026-05-18T01:06:47.366819+00:00"},{"alias_kind":"pith_short_12","alias_value":"5ADJJPSDGAIF","created_at":"2026-05-18T12:25:51.375804+00:00"},{"alias_kind":"pith_short_16","alias_value":"5ADJJPSDGAIFXBAT","created_at":"2026-05-18T12:25:51.375804+00:00"},{"alias_kind":"pith_short_8","alias_value":"5ADJJPSD","created_at":"2026-05-18T12:25:51.375804+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/5ADJJPSDGAIFXBATRWSDHYXKZQ","json":"https://pith.science/pith/5ADJJPSDGAIFXBATRWSDHYXKZQ.json","graph_json":"https://pith.science/api/pith-number/5ADJJPSDGAIFXBATRWSDHYXKZQ/graph.json","events_json":"https://pith.science/api/pith-number/5ADJJPSDGAIFXBATRWSDHYXKZQ/events.json","paper":"https://pith.science/paper/5ADJJPSD"},"agent_actions":{"view_html":"https://pith.science/pith/5ADJJPSDGAIFXBATRWSDHYXKZQ","download_json":"https://pith.science/pith/5ADJJPSDGAIFXBATRWSDHYXKZQ.json","view_paper":"https://pith.science/paper/5ADJJPSD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/0310030&json=true","fetch_graph":"https://pith.science/api/pith-number/5ADJJPSDGAIFXBATRWSDHYXKZQ/graph.json","fetch_events":"https://pith.science/api/pith-number/5ADJJPSDGAIFXBATRWSDHYXKZQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5ADJJPSDGAIFXBATRWSDHYXKZQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5ADJJPSDGAIFXBATRWSDHYXKZQ/action/storage_attestation","attest_author":"https://pith.science/pith/5ADJJPSDGAIFXBATRWSDHYXKZQ/action/author_attestation","sign_citation":"https://pith.science/pith/5ADJJPSDGAIFXBATRWSDHYXKZQ/action/citation_signature","submit_replication":"https://pith.science/pith/5ADJJPSDGAIFXBATRWSDHYXKZQ/action/replication_record"}},"created_at":"2026-05-18T01:06:47.366819+00:00","updated_at":"2026-05-18T01:06:47.366819+00:00"}