{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:KT5OJIHDSGHJBYX7AGRCMFF22K","short_pith_number":"pith:KT5OJIHD","schema_version":"1.0","canonical_sha256":"54fae4a0e3918e90e2ff01a22614bad290f0fd5d5b405a021a1546d4b6fe905f","source":{"kind":"arxiv","id":"1705.10425","version":2},"attestation_state":"computed","paper":{"title":"Rayleigh-Taylor Instability in Two-Component Relativistic Jets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Kenji Toma, Oliver Porth, Serguei S. Komissarov","submitted_at":"2017-05-30T01:30:02Z","abstract_excerpt":"Relativistic jets associated with active galactic nuclei and gamma-ray bursts propagate over huge distances without significant loss of momentum. At the same time they are bright emitters, which is indicative of strong energy dissipation. This points towards a mechanism of internal dissipation which does not result in a global disruption of the flow. One possibility is internal shocks and another one is turbulence driven by local instabilities. Such instabilities can be triggered when a freely expanding jet is reconfined by either the cocoon or external gas pressure. In this paper we study 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":"1705.10425","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-05-30T01:30:02Z","cross_cats_sorted":[],"title_canon_sha256":"900e39db6dda683e219923ac53a8632ae07ee1470963dd37ad72d969ad8ce6bb","abstract_canon_sha256":"3135a7dcff5048ea6af817a1181f52bd6f3d931327bca5081467712637daf419"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:34:48.344261Z","signature_b64":"XWaLpNeKBPnPE8FV3BD4b78ktOLTiQUfRf+LVTXsqHTP14AdJtwByyalPnma5o8xys1opm2iDLZnmI085qHrAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"54fae4a0e3918e90e2ff01a22614bad290f0fd5d5b405a021a1546d4b6fe905f","last_reissued_at":"2026-05-18T00:34:48.343575Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:34:48.343575Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Rayleigh-Taylor Instability in Two-Component Relativistic Jets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Kenji Toma, Oliver Porth, Serguei S. Komissarov","submitted_at":"2017-05-30T01:30:02Z","abstract_excerpt":"Relativistic jets associated with active galactic nuclei and gamma-ray bursts propagate over huge distances without significant loss of momentum. At the same time they are bright emitters, which is indicative of strong energy dissipation. This points towards a mechanism of internal dissipation which does not result in a global disruption of the flow. One possibility is internal shocks and another one is turbulence driven by local instabilities. Such instabilities can be triggered when a freely expanding jet is reconfined by either the cocoon or external gas pressure. In this paper we study the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.10425","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":"1705.10425","created_at":"2026-05-18T00:34:48.343679+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.10425v2","created_at":"2026-05-18T00:34:48.343679+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.10425","created_at":"2026-05-18T00:34:48.343679+00:00"},{"alias_kind":"pith_short_12","alias_value":"KT5OJIHDSGHJ","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_16","alias_value":"KT5OJIHDSGHJBYX7","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_8","alias_value":"KT5OJIHD","created_at":"2026-05-18T12:31:28.150371+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/KT5OJIHDSGHJBYX7AGRCMFF22K","json":"https://pith.science/pith/KT5OJIHDSGHJBYX7AGRCMFF22K.json","graph_json":"https://pith.science/api/pith-number/KT5OJIHDSGHJBYX7AGRCMFF22K/graph.json","events_json":"https://pith.science/api/pith-number/KT5OJIHDSGHJBYX7AGRCMFF22K/events.json","paper":"https://pith.science/paper/KT5OJIHD"},"agent_actions":{"view_html":"https://pith.science/pith/KT5OJIHDSGHJBYX7AGRCMFF22K","download_json":"https://pith.science/pith/KT5OJIHDSGHJBYX7AGRCMFF22K.json","view_paper":"https://pith.science/paper/KT5OJIHD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.10425&json=true","fetch_graph":"https://pith.science/api/pith-number/KT5OJIHDSGHJBYX7AGRCMFF22K/graph.json","fetch_events":"https://pith.science/api/pith-number/KT5OJIHDSGHJBYX7AGRCMFF22K/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KT5OJIHDSGHJBYX7AGRCMFF22K/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KT5OJIHDSGHJBYX7AGRCMFF22K/action/storage_attestation","attest_author":"https://pith.science/pith/KT5OJIHDSGHJBYX7AGRCMFF22K/action/author_attestation","sign_citation":"https://pith.science/pith/KT5OJIHDSGHJBYX7AGRCMFF22K/action/citation_signature","submit_replication":"https://pith.science/pith/KT5OJIHDSGHJBYX7AGRCMFF22K/action/replication_record"}},"created_at":"2026-05-18T00:34:48.343679+00:00","updated_at":"2026-05-18T00:34:48.343679+00:00"}