{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:JKIQPKZRHS2FOZAK42HDJNKP3D","short_pith_number":"pith:JKIQPKZR","schema_version":"1.0","canonical_sha256":"4a9107ab313cb457640ae68e34b54fd8f9a8b60865c4157d547916236abbf83d","source":{"kind":"arxiv","id":"2411.18046","version":3},"attestation_state":"computed","paper":{"title":"Secular evolution of quasi-periodic eruptions","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Cong Zhou, Yuhe Zeng, Zhen Pan","submitted_at":"2024-11-27T04:31:22Z","abstract_excerpt":"Quasi-periodic eruptions (QPEs) are intense repeating soft X-ray bursts with recurrence times about a few hours to a few weeks from galactic nuclei. More and more analyses show that QPEs are the result of collisions between a stellar mass object (SMO, a stellar mass black hole or a main sequence star) and an accretion disk around a supermassive black hole (SMBH) in galactic nuclei. In this work, we propose an osculating trajectory method for efficiently calculating secular evolution of extreme mass ratio inspirals (EMRIs) that are perturbed by an accretion disk. This method accelerates the cal"},"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":"2411.18046","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-11-27T04:31:22Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"326030d821cac603778d90ded9ce6242aa4822602c2865f4c5307c8f8c1f3f6c","abstract_canon_sha256":"c91d264e4b3eccc9c30dc0127c7e67e3b67731c66d0ec8dd442a0b36f969db70"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:51:29.241076Z","signature_b64":"kIsZYDwpP7a1RWzlAN5EUWf3E9sm8UZ30wfkKkR144WLbx+VkX3H3exDWavy94Z7TRP+2/Fa1O1BvgptTUWVCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4a9107ab313cb457640ae68e34b54fd8f9a8b60865c4157d547916236abbf83d","last_reissued_at":"2026-07-05T10:51:29.240562Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:51:29.240562Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Secular evolution of quasi-periodic eruptions","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Cong Zhou, Yuhe Zeng, Zhen Pan","submitted_at":"2024-11-27T04:31:22Z","abstract_excerpt":"Quasi-periodic eruptions (QPEs) are intense repeating soft X-ray bursts with recurrence times about a few hours to a few weeks from galactic nuclei. More and more analyses show that QPEs are the result of collisions between a stellar mass object (SMO, a stellar mass black hole or a main sequence star) and an accretion disk around a supermassive black hole (SMBH) in galactic nuclei. In this work, we propose an osculating trajectory method for efficiently calculating secular evolution of extreme mass ratio inspirals (EMRIs) that are perturbed by an accretion disk. This method accelerates the cal"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.18046","kind":"arxiv","version":3},"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/2411.18046/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":"2411.18046","created_at":"2026-07-05T10:51:29.240622+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.18046v3","created_at":"2026-07-05T10:51:29.240622+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.18046","created_at":"2026-07-05T10:51:29.240622+00:00"},{"alias_kind":"pith_short_12","alias_value":"JKIQPKZRHS2F","created_at":"2026-07-05T10:51:29.240622+00:00"},{"alias_kind":"pith_short_16","alias_value":"JKIQPKZRHS2FOZAK","created_at":"2026-07-05T10:51:29.240622+00:00"},{"alias_kind":"pith_short_8","alias_value":"JKIQPKZR","created_at":"2026-07-05T10:51:29.240622+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.27661","citing_title":"Extreme Mass Ratio Inspirals in Light of Quasi-periodic Eruptions: Milli-Hertz Gravitational Wave Background","ref_index":36,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JKIQPKZRHS2FOZAK42HDJNKP3D","json":"https://pith.science/pith/JKIQPKZRHS2FOZAK42HDJNKP3D.json","graph_json":"https://pith.science/api/pith-number/JKIQPKZRHS2FOZAK42HDJNKP3D/graph.json","events_json":"https://pith.science/api/pith-number/JKIQPKZRHS2FOZAK42HDJNKP3D/events.json","paper":"https://pith.science/paper/JKIQPKZR"},"agent_actions":{"view_html":"https://pith.science/pith/JKIQPKZRHS2FOZAK42HDJNKP3D","download_json":"https://pith.science/pith/JKIQPKZRHS2FOZAK42HDJNKP3D.json","view_paper":"https://pith.science/paper/JKIQPKZR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.18046&json=true","fetch_graph":"https://pith.science/api/pith-number/JKIQPKZRHS2FOZAK42HDJNKP3D/graph.json","fetch_events":"https://pith.science/api/pith-number/JKIQPKZRHS2FOZAK42HDJNKP3D/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JKIQPKZRHS2FOZAK42HDJNKP3D/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JKIQPKZRHS2FOZAK42HDJNKP3D/action/storage_attestation","attest_author":"https://pith.science/pith/JKIQPKZRHS2FOZAK42HDJNKP3D/action/author_attestation","sign_citation":"https://pith.science/pith/JKIQPKZRHS2FOZAK42HDJNKP3D/action/citation_signature","submit_replication":"https://pith.science/pith/JKIQPKZRHS2FOZAK42HDJNKP3D/action/replication_record"}},"created_at":"2026-07-05T10:51:29.240622+00:00","updated_at":"2026-07-05T10:51:29.240622+00:00"}