{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:VEWTY4SX42NF7QYLKUBN7N733V","short_pith_number":"pith:VEWTY4SX","schema_version":"1.0","canonical_sha256":"a92d3c7257e69a5fc30b5502dfb7fbdd40b6d58ea29407752710e833cc4ff3d9","source":{"kind":"arxiv","id":"1212.4810","version":2},"attestation_state":"computed","paper":{"title":"Black hole-neutron star mergers at realistic mass ratios: Equation of state and spin orientation effects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Bela Szilagyi, Christian D. Ott, Francois Foucart, Harald P. Pfeiffer, Ilana MacDonald, Lawrence E. Kidder, Mark A. Scheel, Matthew D. Duez, M. Brett Deaton, Saul A. Teukolsky","submitted_at":"2012-12-19T20:08:25Z","abstract_excerpt":"Black hole-neutron star mergers resulting in the disruption of the neutron star and the formation of an accretion disk and/or the ejection of unbound material are prime candidates for the joint detection of gravitational-wave and electromagnetic signals when the next generation of gravitational-wave detectors comes online. However, the disruption of the neutron star and the properties of the post-merger remnant are very sensitive to the parameters of the binary. In this paper, we study the impact of the radius of the neutron star and the alignment of the black hole spin for systems within the "},"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":"1212.4810","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2012-12-19T20:08:25Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"eb213deeac1f9da4a3e878d0f52e9fa492fa2b6b083334336a0924165d63cda6","abstract_canon_sha256":"420ab5a75b6f7759ab797ced28e7ee59b6fa9fb55a39c0b0849e54d32a593d7e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:27:42.648167Z","signature_b64":"D/+z6rlhE+tIzgLFOWMIWGRq9ylFB4ts+PaywEY7XXsTXy1tVb5qeE1NdVmgzJiHlc2rTiBxuaN+oRWIUsndAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a92d3c7257e69a5fc30b5502dfb7fbdd40b6d58ea29407752710e833cc4ff3d9","last_reissued_at":"2026-05-18T03:27:42.647689Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:27:42.647689Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Black hole-neutron star mergers at realistic mass ratios: Equation of state and spin orientation effects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Bela Szilagyi, Christian D. Ott, Francois Foucart, Harald P. Pfeiffer, Ilana MacDonald, Lawrence E. Kidder, Mark A. Scheel, Matthew D. Duez, M. Brett Deaton, Saul A. Teukolsky","submitted_at":"2012-12-19T20:08:25Z","abstract_excerpt":"Black hole-neutron star mergers resulting in the disruption of the neutron star and the formation of an accretion disk and/or the ejection of unbound material are prime candidates for the joint detection of gravitational-wave and electromagnetic signals when the next generation of gravitational-wave detectors comes online. However, the disruption of the neutron star and the properties of the post-merger remnant are very sensitive to the parameters of the binary. In this paper, we study the impact of the radius of the neutron star and the alignment of the black hole spin for systems within the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1212.4810","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":"1212.4810","created_at":"2026-05-18T03:27:42.647758+00:00"},{"alias_kind":"arxiv_version","alias_value":"1212.4810v2","created_at":"2026-05-18T03:27:42.647758+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1212.4810","created_at":"2026-05-18T03:27:42.647758+00:00"},{"alias_kind":"pith_short_12","alias_value":"VEWTY4SX42NF","created_at":"2026-05-18T12:27:25.539911+00:00"},{"alias_kind":"pith_short_16","alias_value":"VEWTY4SX42NF7QYL","created_at":"2026-05-18T12:27:25.539911+00:00"},{"alias_kind":"pith_short_8","alias_value":"VEWTY4SX","created_at":"2026-05-18T12:27:25.539911+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/VEWTY4SX42NF7QYLKUBN7N733V","json":"https://pith.science/pith/VEWTY4SX42NF7QYLKUBN7N733V.json","graph_json":"https://pith.science/api/pith-number/VEWTY4SX42NF7QYLKUBN7N733V/graph.json","events_json":"https://pith.science/api/pith-number/VEWTY4SX42NF7QYLKUBN7N733V/events.json","paper":"https://pith.science/paper/VEWTY4SX"},"agent_actions":{"view_html":"https://pith.science/pith/VEWTY4SX42NF7QYLKUBN7N733V","download_json":"https://pith.science/pith/VEWTY4SX42NF7QYLKUBN7N733V.json","view_paper":"https://pith.science/paper/VEWTY4SX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1212.4810&json=true","fetch_graph":"https://pith.science/api/pith-number/VEWTY4SX42NF7QYLKUBN7N733V/graph.json","fetch_events":"https://pith.science/api/pith-number/VEWTY4SX42NF7QYLKUBN7N733V/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VEWTY4SX42NF7QYLKUBN7N733V/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VEWTY4SX42NF7QYLKUBN7N733V/action/storage_attestation","attest_author":"https://pith.science/pith/VEWTY4SX42NF7QYLKUBN7N733V/action/author_attestation","sign_citation":"https://pith.science/pith/VEWTY4SX42NF7QYLKUBN7N733V/action/citation_signature","submit_replication":"https://pith.science/pith/VEWTY4SX42NF7QYLKUBN7N733V/action/replication_record"}},"created_at":"2026-05-18T03:27:42.647758+00:00","updated_at":"2026-05-18T03:27:42.647758+00:00"}