{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:XTMUNK3AR3X3ZBZFL52WR6KRW2","short_pith_number":"pith:XTMUNK3A","schema_version":"1.0","canonical_sha256":"bcd946ab608eefbc87255f7568f951b6beffae2371918f77bacc6f972b429f59","source":{"kind":"arxiv","id":"2308.05161","version":1},"attestation_state":"computed","paper":{"title":"A Unified Theory of Jetted Tidal Disruption Events: From Promptly Escaping Relativistic to Delayed Transrelativistic Jets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Brian D. Metzger, Odelia Teboul","submitted_at":"2023-08-09T18:05:49Z","abstract_excerpt":"Only a tiny fraction ~ 1% of stellar tidal disruption events (TDE) generate powerful relativistic jets evidenced by luminous hard X-ray and radio emissions. We propose that a key property responsible for both this surprisingly low rate and a variety of other observations is the typically large misalignment {\\psi} between the orbital plane of the star and the spin axis of the supermassive black hole (SMBH). Such misaligned disk/jet systems undergo Lense-Thirring precession together about the SMBH spin axis. We find that TDE disks precess sufficiently rapidly that winds from the accretion disk w"},"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":"2308.05161","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-08-09T18:05:49Z","cross_cats_sorted":[],"title_canon_sha256":"0085bef5525fd175badbad0fd302043c001614f2575b4a74ae3a55a0e304ac5b","abstract_canon_sha256":"c6e198f9969a52da9d07170e7737c5f4253dddecad944b5a317cc3c5624d194d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:39:56.509807Z","signature_b64":"T5vjb47LY6ls6DAOr01ySgWW8e61gbHlyHg/5KOSbs0A4B31nZbIJLUNUN/Jf+0TG8cvpCwxqedtR1aNiNafCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bcd946ab608eefbc87255f7568f951b6beffae2371918f77bacc6f972b429f59","last_reissued_at":"2026-07-05T06:39:56.509345Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:39:56.509345Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Unified Theory of Jetted Tidal Disruption Events: From Promptly Escaping Relativistic to Delayed Transrelativistic Jets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Brian D. Metzger, Odelia Teboul","submitted_at":"2023-08-09T18:05:49Z","abstract_excerpt":"Only a tiny fraction ~ 1% of stellar tidal disruption events (TDE) generate powerful relativistic jets evidenced by luminous hard X-ray and radio emissions. We propose that a key property responsible for both this surprisingly low rate and a variety of other observations is the typically large misalignment {\\psi} between the orbital plane of the star and the spin axis of the supermassive black hole (SMBH). Such misaligned disk/jet systems undergo Lense-Thirring precession together about the SMBH spin axis. We find that TDE disks precess sufficiently rapidly that winds from the accretion disk w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2308.05161","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2308.05161/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":"2308.05161","created_at":"2026-07-05T06:39:56.509422+00:00"},{"alias_kind":"arxiv_version","alias_value":"2308.05161v1","created_at":"2026-07-05T06:39:56.509422+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2308.05161","created_at":"2026-07-05T06:39:56.509422+00:00"},{"alias_kind":"pith_short_12","alias_value":"XTMUNK3AR3X3","created_at":"2026-07-05T06:39:56.509422+00:00"},{"alias_kind":"pith_short_16","alias_value":"XTMUNK3AR3X3ZBZF","created_at":"2026-07-05T06:39:56.509422+00:00"},{"alias_kind":"pith_short_8","alias_value":"XTMUNK3A","created_at":"2026-07-05T06:39:56.509422+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.08090","citing_title":"Multi-wavelength Constraints on the Transient EP250905a","ref_index":149,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XTMUNK3AR3X3ZBZFL52WR6KRW2","json":"https://pith.science/pith/XTMUNK3AR3X3ZBZFL52WR6KRW2.json","graph_json":"https://pith.science/api/pith-number/XTMUNK3AR3X3ZBZFL52WR6KRW2/graph.json","events_json":"https://pith.science/api/pith-number/XTMUNK3AR3X3ZBZFL52WR6KRW2/events.json","paper":"https://pith.science/paper/XTMUNK3A"},"agent_actions":{"view_html":"https://pith.science/pith/XTMUNK3AR3X3ZBZFL52WR6KRW2","download_json":"https://pith.science/pith/XTMUNK3AR3X3ZBZFL52WR6KRW2.json","view_paper":"https://pith.science/paper/XTMUNK3A","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2308.05161&json=true","fetch_graph":"https://pith.science/api/pith-number/XTMUNK3AR3X3ZBZFL52WR6KRW2/graph.json","fetch_events":"https://pith.science/api/pith-number/XTMUNK3AR3X3ZBZFL52WR6KRW2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XTMUNK3AR3X3ZBZFL52WR6KRW2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XTMUNK3AR3X3ZBZFL52WR6KRW2/action/storage_attestation","attest_author":"https://pith.science/pith/XTMUNK3AR3X3ZBZFL52WR6KRW2/action/author_attestation","sign_citation":"https://pith.science/pith/XTMUNK3AR3X3ZBZFL52WR6KRW2/action/citation_signature","submit_replication":"https://pith.science/pith/XTMUNK3AR3X3ZBZFL52WR6KRW2/action/replication_record"}},"created_at":"2026-07-05T06:39:56.509422+00:00","updated_at":"2026-07-05T06:39:56.509422+00:00"}