{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:4CQVBVAB6HG7RN23SMWONRBQ7S","short_pith_number":"pith:4CQVBVAB","schema_version":"1.0","canonical_sha256":"e0a150d401f1cdf8b75b932ce6c430fcb9cc3ad088dce751f982d3ec1605b94b","source":{"kind":"arxiv","id":"2305.00036","version":2},"attestation_state":"computed","paper":{"title":"Linear analysis of the Kelvin-Helmholtz instability in relativistic magnetized symmetric flows","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Anthony Chow, Gianluigi Bodo, Jordy Davelaar, Lorenzo Sironi, Michael E. Rowan, Ramesh Narayan","submitted_at":"2023-04-28T18:20:16Z","abstract_excerpt":"We study the linear stability of a planar interface separating two fluids in relative motion, focusing on the symmetric configuration where the two fluids have the same properties (density, temperature, magnetic field strength, and direction). We consider the most general case with arbitrary sound speed $c_{\\rm s}$, Alfv\\'en speed $v_{\\rm A}$, and magnetic field orientation. For the instability associated with the fast mode, we find that the lower bound of unstable shear velocities is set by the requirement that the projection of the velocity onto the fluid-frame wavevector is larger than 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":"2305.00036","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-04-28T18:20:16Z","cross_cats_sorted":[],"title_canon_sha256":"27a84806b344f0090b1d9d7ad2598fe96cf7d7cb63931e5fbd7be6a8bb01ef1a","abstract_canon_sha256":"bf8fc59e7ad4621b88961f029a2387903df75f008f1388c3f2901a320ba8e6c7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:28:17.968890Z","signature_b64":"fkv+T5Atrs1DB0Kq2VWsdrQ6E5cDPFbYbOEPoRt547oGX7M2xwFB0DUma774g1mpgsDPZ32IXqqBl1lNQKFIAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e0a150d401f1cdf8b75b932ce6c430fcb9cc3ad088dce751f982d3ec1605b94b","last_reissued_at":"2026-07-05T06:28:17.968491Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:28:17.968491Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Linear analysis of the Kelvin-Helmholtz instability in relativistic magnetized symmetric flows","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Anthony Chow, Gianluigi Bodo, Jordy Davelaar, Lorenzo Sironi, Michael E. Rowan, Ramesh Narayan","submitted_at":"2023-04-28T18:20:16Z","abstract_excerpt":"We study the linear stability of a planar interface separating two fluids in relative motion, focusing on the symmetric configuration where the two fluids have the same properties (density, temperature, magnetic field strength, and direction). We consider the most general case with arbitrary sound speed $c_{\\rm s}$, Alfv\\'en speed $v_{\\rm A}$, and magnetic field orientation. For the instability associated with the fast mode, we find that the lower bound of unstable shear velocities is set by the requirement that the projection of the velocity onto the fluid-frame wavevector is larger than the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2305.00036","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/2305.00036/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":"2305.00036","created_at":"2026-07-05T06:28:17.968550+00:00"},{"alias_kind":"arxiv_version","alias_value":"2305.00036v2","created_at":"2026-07-05T06:28:17.968550+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2305.00036","created_at":"2026-07-05T06:28:17.968550+00:00"},{"alias_kind":"pith_short_12","alias_value":"4CQVBVAB6HG7","created_at":"2026-07-05T06:28:17.968550+00:00"},{"alias_kind":"pith_short_16","alias_value":"4CQVBVAB6HG7RN23","created_at":"2026-07-05T06:28:17.968550+00:00"},{"alias_kind":"pith_short_8","alias_value":"4CQVBVAB","created_at":"2026-07-05T06:28:17.968550+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.10708","citing_title":"Classical waves and instabilities using the minimalist approach","ref_index":12,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4CQVBVAB6HG7RN23SMWONRBQ7S","json":"https://pith.science/pith/4CQVBVAB6HG7RN23SMWONRBQ7S.json","graph_json":"https://pith.science/api/pith-number/4CQVBVAB6HG7RN23SMWONRBQ7S/graph.json","events_json":"https://pith.science/api/pith-number/4CQVBVAB6HG7RN23SMWONRBQ7S/events.json","paper":"https://pith.science/paper/4CQVBVAB"},"agent_actions":{"view_html":"https://pith.science/pith/4CQVBVAB6HG7RN23SMWONRBQ7S","download_json":"https://pith.science/pith/4CQVBVAB6HG7RN23SMWONRBQ7S.json","view_paper":"https://pith.science/paper/4CQVBVAB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2305.00036&json=true","fetch_graph":"https://pith.science/api/pith-number/4CQVBVAB6HG7RN23SMWONRBQ7S/graph.json","fetch_events":"https://pith.science/api/pith-number/4CQVBVAB6HG7RN23SMWONRBQ7S/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4CQVBVAB6HG7RN23SMWONRBQ7S/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4CQVBVAB6HG7RN23SMWONRBQ7S/action/storage_attestation","attest_author":"https://pith.science/pith/4CQVBVAB6HG7RN23SMWONRBQ7S/action/author_attestation","sign_citation":"https://pith.science/pith/4CQVBVAB6HG7RN23SMWONRBQ7S/action/citation_signature","submit_replication":"https://pith.science/pith/4CQVBVAB6HG7RN23SMWONRBQ7S/action/replication_record"}},"created_at":"2026-07-05T06:28:17.968550+00:00","updated_at":"2026-07-05T06:28:17.968550+00:00"}