{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:35MCDIMYZQUOEXEP2D7TNH4CBG","short_pith_number":"pith:35MCDIMY","schema_version":"1.0","canonical_sha256":"df5821a198cc28e25c8fd0ff369f8209b07073c5a127f220b5828593a547cc23","source":{"kind":"arxiv","id":"1602.05763","version":1},"attestation_state":"computed","paper":{"title":"Stellar Dynamics around a Massive Black Hole III: Resonant Relaxation of Axisymmetric Discs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Jihad R. Touma, S. Sridhar","submitted_at":"2016-02-18T11:34:43Z","abstract_excerpt":"We study the Resonant Relaxation (RR) of an axisymmetric low mass (or Keplerian) stellar disc orbiting a more massive black hole (MBH). Our recent work on the general kinetic theory of RR is simplified in the standard manner by ignoring the effects of `gravitational polarization', and applied to a zero-thickness, flat, axisymmetric disc. The wake of a stellar orbit is expressed in terms of the angular momenta exchanged with other orbits, and used to derive a kinetic equation for RR under the combined actions of self-gravity, 1 PN and 1.5 PN relativistic effects of the MBH and an arbitrary exte"},"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":"1602.05763","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-02-18T11:34:43Z","cross_cats_sorted":[],"title_canon_sha256":"38ae34f4b2d2e510990c1e1e069ec023eb3e3334df9db825181842337e10b9ef","abstract_canon_sha256":"cef48e42b35ead6a273d130089d9560737318ab202c9de631f2e2d3ef42d4e3c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:54:40.746536Z","signature_b64":"6U7c4ZSVwEdd6oLZ9GKEkLjGZlRmOkhsRdHyqt0hLe+Ng54E86HdtKNUWY+Sq1gWkNcAXwKC2nbefxZ9o9ZhBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"df5821a198cc28e25c8fd0ff369f8209b07073c5a127f220b5828593a547cc23","last_reissued_at":"2026-05-18T00:54:40.745810Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:54:40.745810Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stellar Dynamics around a Massive Black Hole III: Resonant Relaxation of Axisymmetric Discs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Jihad R. Touma, S. Sridhar","submitted_at":"2016-02-18T11:34:43Z","abstract_excerpt":"We study the Resonant Relaxation (RR) of an axisymmetric low mass (or Keplerian) stellar disc orbiting a more massive black hole (MBH). Our recent work on the general kinetic theory of RR is simplified in the standard manner by ignoring the effects of `gravitational polarization', and applied to a zero-thickness, flat, axisymmetric disc. The wake of a stellar orbit is expressed in terms of the angular momenta exchanged with other orbits, and used to derive a kinetic equation for RR under the combined actions of self-gravity, 1 PN and 1.5 PN relativistic effects of the MBH and an arbitrary exte"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.05763","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":""},"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":"1602.05763","created_at":"2026-05-18T00:54:40.745938+00:00"},{"alias_kind":"arxiv_version","alias_value":"1602.05763v1","created_at":"2026-05-18T00:54:40.745938+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1602.05763","created_at":"2026-05-18T00:54:40.745938+00:00"},{"alias_kind":"pith_short_12","alias_value":"35MCDIMYZQUO","created_at":"2026-05-18T12:29:55.572404+00:00"},{"alias_kind":"pith_short_16","alias_value":"35MCDIMYZQUOEXEP","created_at":"2026-05-18T12:29:55.572404+00:00"},{"alias_kind":"pith_short_8","alias_value":"35MCDIMY","created_at":"2026-05-18T12:29:55.572404+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/35MCDIMYZQUOEXEP2D7TNH4CBG","json":"https://pith.science/pith/35MCDIMYZQUOEXEP2D7TNH4CBG.json","graph_json":"https://pith.science/api/pith-number/35MCDIMYZQUOEXEP2D7TNH4CBG/graph.json","events_json":"https://pith.science/api/pith-number/35MCDIMYZQUOEXEP2D7TNH4CBG/events.json","paper":"https://pith.science/paper/35MCDIMY"},"agent_actions":{"view_html":"https://pith.science/pith/35MCDIMYZQUOEXEP2D7TNH4CBG","download_json":"https://pith.science/pith/35MCDIMYZQUOEXEP2D7TNH4CBG.json","view_paper":"https://pith.science/paper/35MCDIMY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1602.05763&json=true","fetch_graph":"https://pith.science/api/pith-number/35MCDIMYZQUOEXEP2D7TNH4CBG/graph.json","fetch_events":"https://pith.science/api/pith-number/35MCDIMYZQUOEXEP2D7TNH4CBG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/35MCDIMYZQUOEXEP2D7TNH4CBG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/35MCDIMYZQUOEXEP2D7TNH4CBG/action/storage_attestation","attest_author":"https://pith.science/pith/35MCDIMYZQUOEXEP2D7TNH4CBG/action/author_attestation","sign_citation":"https://pith.science/pith/35MCDIMYZQUOEXEP2D7TNH4CBG/action/citation_signature","submit_replication":"https://pith.science/pith/35MCDIMYZQUOEXEP2D7TNH4CBG/action/replication_record"}},"created_at":"2026-05-18T00:54:40.745938+00:00","updated_at":"2026-05-18T00:54:40.745938+00:00"}