{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:OZE2UN3CDPU23QWYNZOGC5K46G","short_pith_number":"pith:OZE2UN3C","schema_version":"1.0","canonical_sha256":"7649aa37621be9adc2d86e5c61755cf1ac95e14dc238b1059bd7adc2f968c252","source":{"kind":"arxiv","id":"2104.01208","version":2},"attestation_state":"computed","paper":{"title":"Wet Extreme Mass Ratio Inspirals May Be More Common For Spaceborne Gravitational Wave Detection","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Huan Yang, Zhen Pan, Zhenwei Lyu","submitted_at":"2021-04-02T19:17:10Z","abstract_excerpt":"Extreme Mass Ratio Inspirals (EMRIs) can be classified as dry EMRIs and wet EMRIs based on their formation mechanisms. Dry (or the \"loss-cone\") EMRIs, previously considered as the main EMRI sources for the Laser Interferometer Space Antenna, are primarily produced by multi-body scattering in the nuclear star cluster and gravitational capture. In this work, we highlight an alternative EMRI formation channel: (wet) EMRI formation assisted by the accretion flow around accreting galactic-center massive black holes (MBHs). In this channel, the accretion disk captures stellar-mass black holes that a"},"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":"2104.01208","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2021-04-02T19:17:10Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"f0da76d006da991954fadf6b32a6e2ac9e527f0adcf6726940e66cde2af3171a","abstract_canon_sha256":"7d4525239b227111ca89f360b32ce2f52e97929bde4ac8afebc2c8b4f2e1a2b7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:12:02.295206Z","signature_b64":"yHMWIFGAHdGmT32//e0ClJYWt6N9F/vkWM/4aUwwPX0W8nvWph4GAfcyfWsyBNnf8DlnOeVbKy6ttvt0C7dJCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7649aa37621be9adc2d86e5c61755cf1ac95e14dc238b1059bd7adc2f968c252","last_reissued_at":"2026-07-05T03:12:02.294766Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:12:02.294766Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Wet Extreme Mass Ratio Inspirals May Be More Common For Spaceborne Gravitational Wave Detection","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Huan Yang, Zhen Pan, Zhenwei Lyu","submitted_at":"2021-04-02T19:17:10Z","abstract_excerpt":"Extreme Mass Ratio Inspirals (EMRIs) can be classified as dry EMRIs and wet EMRIs based on their formation mechanisms. Dry (or the \"loss-cone\") EMRIs, previously considered as the main EMRI sources for the Laser Interferometer Space Antenna, are primarily produced by multi-body scattering in the nuclear star cluster and gravitational capture. In this work, we highlight an alternative EMRI formation channel: (wet) EMRI formation assisted by the accretion flow around accreting galactic-center massive black holes (MBHs). In this channel, the accretion disk captures stellar-mass black holes that a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2104.01208","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/2104.01208/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":"2104.01208","created_at":"2026-07-05T03:12:02.294823+00:00"},{"alias_kind":"arxiv_version","alias_value":"2104.01208v2","created_at":"2026-07-05T03:12:02.294823+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2104.01208","created_at":"2026-07-05T03:12:02.294823+00:00"},{"alias_kind":"pith_short_12","alias_value":"OZE2UN3CDPU2","created_at":"2026-07-05T03:12:02.294823+00:00"},{"alias_kind":"pith_short_16","alias_value":"OZE2UN3CDPU23QWY","created_at":"2026-07-05T03:12:02.294823+00:00"},{"alias_kind":"pith_short_8","alias_value":"OZE2UN3C","created_at":"2026-07-05T03:12:02.294823+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.05909","citing_title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","ref_index":29,"is_internal_anchor":true},{"citing_arxiv_id":"2606.27526","citing_title":"Dynamics of Relativistic Binaries in Structured and Stochastic Environments: A Lagrange-Fourier-Hansen Framework","ref_index":168,"is_internal_anchor":false},{"citing_arxiv_id":"2311.01300","citing_title":"Waveform Modelling for the Laser Interferometer Space Antenna","ref_index":80,"is_internal_anchor":false},{"citing_arxiv_id":"2508.16399","citing_title":"Constraints on the extreme mass-ratio inspiral population from LISA data","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2604.10942","citing_title":"Probing Active Galactic Nuclei and Measuring the Hubble constant with Extreme-Mass-Ratio Inspirals","ref_index":13,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06053","citing_title":"Probing Kerr Symmetry Breaking with LISA Extreme-Mass-Ratio Inspirals","ref_index":41,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OZE2UN3CDPU23QWYNZOGC5K46G","json":"https://pith.science/pith/OZE2UN3CDPU23QWYNZOGC5K46G.json","graph_json":"https://pith.science/api/pith-number/OZE2UN3CDPU23QWYNZOGC5K46G/graph.json","events_json":"https://pith.science/api/pith-number/OZE2UN3CDPU23QWYNZOGC5K46G/events.json","paper":"https://pith.science/paper/OZE2UN3C"},"agent_actions":{"view_html":"https://pith.science/pith/OZE2UN3CDPU23QWYNZOGC5K46G","download_json":"https://pith.science/pith/OZE2UN3CDPU23QWYNZOGC5K46G.json","view_paper":"https://pith.science/paper/OZE2UN3C","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2104.01208&json=true","fetch_graph":"https://pith.science/api/pith-number/OZE2UN3CDPU23QWYNZOGC5K46G/graph.json","fetch_events":"https://pith.science/api/pith-number/OZE2UN3CDPU23QWYNZOGC5K46G/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OZE2UN3CDPU23QWYNZOGC5K46G/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OZE2UN3CDPU23QWYNZOGC5K46G/action/storage_attestation","attest_author":"https://pith.science/pith/OZE2UN3CDPU23QWYNZOGC5K46G/action/author_attestation","sign_citation":"https://pith.science/pith/OZE2UN3CDPU23QWYNZOGC5K46G/action/citation_signature","submit_replication":"https://pith.science/pith/OZE2UN3CDPU23QWYNZOGC5K46G/action/replication_record"}},"created_at":"2026-07-05T03:12:02.294823+00:00","updated_at":"2026-07-05T03:12:02.294823+00:00"}