{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:ABVF5WUI5I3Z3NRWBVPXMLWLA6","short_pith_number":"pith:ABVF5WUI","schema_version":"1.0","canonical_sha256":"006a5eda88ea379db6360d5f762ecb079e40b577def88f96d17be777c38a51c0","source":{"kind":"arxiv","id":"2403.09770","version":2},"attestation_state":"computed","paper":{"title":"Large Eddy Simulations of Magnetized Mergers of Black Holes and Neutron Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Carlos Palenzuela, Manuel R. Izquierdo, Miguel Bezares, Steven Liebling","submitted_at":"2024-03-14T18:00:00Z","abstract_excerpt":"The LIGO-Virgo-Kagra collaboration has observed gravitational waves consistent with the mergers of a black hole and a neutron star, namely GW200105 and GW200115, providing evidence for such cataclysmic events. Although no electromagnetic counterpart was reported for either of these two events, under certain conditions black hole--neutron star mergers are expected to form a significant accretion disk and to produce both a short gamma ray burst and a kilonova, much as observed in the binary neutron star merger GW170817. Here, we extend our publicly available code $\\texttt{MHDuet}$ to study numer"},"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":"2403.09770","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-03-14T18:00:00Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"d75660bf691f0abcd46bb3a647173624e14ddb834e5560fb823ac955906b8913","abstract_canon_sha256":"e18d28b3534fd3ac13fc3558502abbb836ee0a4501aca185e73b11771e0bb652"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:15:30.623325Z","signature_b64":"SMVR/GTqCKrK2oX/eTY1aKH/2sRwGb9LH6hWghr2dZZivwyoCnrsKm/GyxFzNdlPC3vZXrmAmX8tcs2f70iLCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"006a5eda88ea379db6360d5f762ecb079e40b577def88f96d17be777c38a51c0","last_reissued_at":"2026-07-05T09:15:30.622621Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:15:30.622621Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Large Eddy Simulations of Magnetized Mergers of Black Holes and Neutron Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Carlos Palenzuela, Manuel R. Izquierdo, Miguel Bezares, Steven Liebling","submitted_at":"2024-03-14T18:00:00Z","abstract_excerpt":"The LIGO-Virgo-Kagra collaboration has observed gravitational waves consistent with the mergers of a black hole and a neutron star, namely GW200105 and GW200115, providing evidence for such cataclysmic events. Although no electromagnetic counterpart was reported for either of these two events, under certain conditions black hole--neutron star mergers are expected to form a significant accretion disk and to produce both a short gamma ray burst and a kilonova, much as observed in the binary neutron star merger GW170817. Here, we extend our publicly available code $\\texttt{MHDuet}$ to study numer"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.09770","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2403.09770/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":"2403.09770","created_at":"2026-07-05T09:15:30.622695+00:00"},{"alias_kind":"arxiv_version","alias_value":"2403.09770v2","created_at":"2026-07-05T09:15:30.622695+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2403.09770","created_at":"2026-07-05T09:15:30.622695+00:00"},{"alias_kind":"pith_short_12","alias_value":"ABVF5WUI5I3Z","created_at":"2026-07-05T09:15:30.622695+00:00"},{"alias_kind":"pith_short_16","alias_value":"ABVF5WUI5I3Z3NRW","created_at":"2026-07-05T09:15:30.622695+00:00"},{"alias_kind":"pith_short_8","alias_value":"ABVF5WUI","created_at":"2026-07-05T09:15:30.622695+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.13154","citing_title":"Implications of Magnetic Flux-Disk Mass Correlation in Black Hole-Neutron Star Mergers for GRB sub-populations","ref_index":36,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ABVF5WUI5I3Z3NRWBVPXMLWLA6","json":"https://pith.science/pith/ABVF5WUI5I3Z3NRWBVPXMLWLA6.json","graph_json":"https://pith.science/api/pith-number/ABVF5WUI5I3Z3NRWBVPXMLWLA6/graph.json","events_json":"https://pith.science/api/pith-number/ABVF5WUI5I3Z3NRWBVPXMLWLA6/events.json","paper":"https://pith.science/paper/ABVF5WUI"},"agent_actions":{"view_html":"https://pith.science/pith/ABVF5WUI5I3Z3NRWBVPXMLWLA6","download_json":"https://pith.science/pith/ABVF5WUI5I3Z3NRWBVPXMLWLA6.json","view_paper":"https://pith.science/paper/ABVF5WUI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2403.09770&json=true","fetch_graph":"https://pith.science/api/pith-number/ABVF5WUI5I3Z3NRWBVPXMLWLA6/graph.json","fetch_events":"https://pith.science/api/pith-number/ABVF5WUI5I3Z3NRWBVPXMLWLA6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ABVF5WUI5I3Z3NRWBVPXMLWLA6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ABVF5WUI5I3Z3NRWBVPXMLWLA6/action/storage_attestation","attest_author":"https://pith.science/pith/ABVF5WUI5I3Z3NRWBVPXMLWLA6/action/author_attestation","sign_citation":"https://pith.science/pith/ABVF5WUI5I3Z3NRWBVPXMLWLA6/action/citation_signature","submit_replication":"https://pith.science/pith/ABVF5WUI5I3Z3NRWBVPXMLWLA6/action/replication_record"}},"created_at":"2026-07-05T09:15:30.622695+00:00","updated_at":"2026-07-05T09:15:30.622695+00:00"}