{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:QWWKFGX4HRKDESVKDLHY334SOX","short_pith_number":"pith:QWWKFGX4","schema_version":"1.0","canonical_sha256":"85aca29afc3c54324aaa1acf8def9275e239dd132b911d072e1292b69a229bd1","source":{"kind":"arxiv","id":"1101.4298","version":2},"attestation_state":"computed","paper":{"title":"The missing link: Merging neutron stars naturally produce jet-like structures and can power short Gamma-Ray Bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.SR","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Bruno Giacomazzo, Chryssa Kouveliotou, Jonathan Granot, Luca Baiotti, Luciano Rezzolla, Miguel A. Aloy","submitted_at":"2011-01-22T15:51:37Z","abstract_excerpt":"Short Gamma-Ray Bursts (SGRBs) are among the most luminous explosions in the universe, releasing in less than one second the energy emitted by our Galaxy over one year. Despite decades of observations, the nature of their \"central-engine\" remains unknown. Considering a binary of magnetized neutron stars and solving Einstein equations, we show that their merger results in a rapidly spinning black hole surrounded by a hot and highly magnetized torus. Lasting over 35 ms and much longer than previous simulations, our study reveals that magnetohydrodynamical instabilities amplify an initially turbu"},"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":"1101.4298","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-01-22T15:51:37Z","cross_cats_sorted":["astro-ph.CO","astro-ph.SR","gr-qc"],"title_canon_sha256":"65cf0c54b9cc2d818452edd1cba66e81e6efa24a0e13f715884e591ebac7de01","abstract_canon_sha256":"8f0e971aeb53f5e663f78c4e68d61d6d68aea55e803d7969331e32dfdbe73025"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:25.351472Z","signature_b64":"kuCtepFGe8AdIdVjChe3F8+8kvbDOqJBDIygg5iMm4OfKTKf0ZF5VUNTqyKPb2Z5tAGkIrBbJ5tB1vpM5Z8ZBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"85aca29afc3c54324aaa1acf8def9275e239dd132b911d072e1292b69a229bd1","last_reissued_at":"2026-05-18T02:03:25.350642Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:25.350642Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The missing link: Merging neutron stars naturally produce jet-like structures and can power short Gamma-Ray Bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.SR","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Bruno Giacomazzo, Chryssa Kouveliotou, Jonathan Granot, Luca Baiotti, Luciano Rezzolla, Miguel A. Aloy","submitted_at":"2011-01-22T15:51:37Z","abstract_excerpt":"Short Gamma-Ray Bursts (SGRBs) are among the most luminous explosions in the universe, releasing in less than one second the energy emitted by our Galaxy over one year. Despite decades of observations, the nature of their \"central-engine\" remains unknown. Considering a binary of magnetized neutron stars and solving Einstein equations, we show that their merger results in a rapidly spinning black hole surrounded by a hot and highly magnetized torus. Lasting over 35 ms and much longer than previous simulations, our study reveals that magnetohydrodynamical instabilities amplify an initially turbu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.4298","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":"1101.4298","created_at":"2026-05-18T02:03:25.350778+00:00"},{"alias_kind":"arxiv_version","alias_value":"1101.4298v2","created_at":"2026-05-18T02:03:25.350778+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.4298","created_at":"2026-05-18T02:03:25.350778+00:00"},{"alias_kind":"pith_short_12","alias_value":"QWWKFGX4HRKD","created_at":"2026-05-18T12:26:39.201973+00:00"},{"alias_kind":"pith_short_16","alias_value":"QWWKFGX4HRKDESVK","created_at":"2026-05-18T12:26:39.201973+00:00"},{"alias_kind":"pith_short_8","alias_value":"QWWKFGX4","created_at":"2026-05-18T12:26:39.201973+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.01337","citing_title":"A possible high-redshift origin for the short GRB 061201: implications of a compact binary merger beyond cosmic noon","ref_index":70,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QWWKFGX4HRKDESVKDLHY334SOX","json":"https://pith.science/pith/QWWKFGX4HRKDESVKDLHY334SOX.json","graph_json":"https://pith.science/api/pith-number/QWWKFGX4HRKDESVKDLHY334SOX/graph.json","events_json":"https://pith.science/api/pith-number/QWWKFGX4HRKDESVKDLHY334SOX/events.json","paper":"https://pith.science/paper/QWWKFGX4"},"agent_actions":{"view_html":"https://pith.science/pith/QWWKFGX4HRKDESVKDLHY334SOX","download_json":"https://pith.science/pith/QWWKFGX4HRKDESVKDLHY334SOX.json","view_paper":"https://pith.science/paper/QWWKFGX4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1101.4298&json=true","fetch_graph":"https://pith.science/api/pith-number/QWWKFGX4HRKDESVKDLHY334SOX/graph.json","fetch_events":"https://pith.science/api/pith-number/QWWKFGX4HRKDESVKDLHY334SOX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QWWKFGX4HRKDESVKDLHY334SOX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QWWKFGX4HRKDESVKDLHY334SOX/action/storage_attestation","attest_author":"https://pith.science/pith/QWWKFGX4HRKDESVKDLHY334SOX/action/author_attestation","sign_citation":"https://pith.science/pith/QWWKFGX4HRKDESVKDLHY334SOX/action/citation_signature","submit_replication":"https://pith.science/pith/QWWKFGX4HRKDESVKDLHY334SOX/action/replication_record"}},"created_at":"2026-05-18T02:03:25.350778+00:00","updated_at":"2026-05-18T02:03:25.350778+00:00"}