{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:5SNO5XU2ERSRMQI6N6BYDFBBSY","short_pith_number":"pith:5SNO5XU2","schema_version":"1.0","canonical_sha256":"ec9aeede9a246516411e6f838194219632fe7f13cfc77744136c9baa1f08b697","source":{"kind":"arxiv","id":"2205.04808","version":1},"attestation_state":"computed","paper":{"title":"Modeling transient resonances in extreme-mass-ratio inspirals","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Alvin J.K. Chua, B\\'eatrice Bonga, Lorenzo Speri, Priti Gupta, Takahiro Tanaka","submitted_at":"2022-05-10T11:18:18Z","abstract_excerpt":"Extreme-mass-ratio inspirals are one of the most exciting and promising target sources for space-based interferometers (such as LISA, TianQin). The observation of their emitted gravitational waves will offer stringent tests on general theory of relativity, and provide a wealth of information about the dense environment in galactic centers. To unlock such potential, it is necessary to correctly characterize EMRI signals. However, resonances are a phenomena that occurs in EMRI systems and can impact parameter inference, and therefore the science outcome, if not properly modeled. Here, we explore"},"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":"2205.04808","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2022-05-10T11:18:18Z","cross_cats_sorted":[],"title_canon_sha256":"cf36cf175d90b60487539be20d2887efd1ba9d03803a69d33eabec5d302ef5f2","abstract_canon_sha256":"64cc6642d7566504386ebea786154e090c8a229e738e053a38f085c6868da2bc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:11:31.806792Z","signature_b64":"YhaW2Pz+SrAXxVqNKMwMnS8w+QqMhKr0ZV9K4jk3rRvQQXKcYn742n2hEPEFSTqv4nIWHLPj8tiahNhc+OX8Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ec9aeede9a246516411e6f838194219632fe7f13cfc77744136c9baa1f08b697","last_reissued_at":"2026-07-05T06:11:31.806307Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:11:31.806307Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Modeling transient resonances in extreme-mass-ratio inspirals","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Alvin J.K. Chua, B\\'eatrice Bonga, Lorenzo Speri, Priti Gupta, Takahiro Tanaka","submitted_at":"2022-05-10T11:18:18Z","abstract_excerpt":"Extreme-mass-ratio inspirals are one of the most exciting and promising target sources for space-based interferometers (such as LISA, TianQin). The observation of their emitted gravitational waves will offer stringent tests on general theory of relativity, and provide a wealth of information about the dense environment in galactic centers. To unlock such potential, it is necessary to correctly characterize EMRI signals. However, resonances are a phenomena that occurs in EMRI systems and can impact parameter inference, and therefore the science outcome, if not properly modeled. Here, we explore"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2205.04808","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2205.04808/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":"2205.04808","created_at":"2026-07-05T06:11:31.806379+00:00"},{"alias_kind":"arxiv_version","alias_value":"2205.04808v1","created_at":"2026-07-05T06:11:31.806379+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2205.04808","created_at":"2026-07-05T06:11:31.806379+00:00"},{"alias_kind":"pith_short_12","alias_value":"5SNO5XU2ERSR","created_at":"2026-07-05T06:11:31.806379+00:00"},{"alias_kind":"pith_short_16","alias_value":"5SNO5XU2ERSRMQI6","created_at":"2026-07-05T06:11:31.806379+00:00"},{"alias_kind":"pith_short_8","alias_value":"5SNO5XU2","created_at":"2026-07-05T06:11:31.806379+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.27526","citing_title":"Dynamics of Relativistic Binaries in Structured and Stochastic Environments: A Lagrange-Fourier-Hansen Framework","ref_index":200,"is_internal_anchor":false},{"citing_arxiv_id":"2311.01300","citing_title":"Waveform Modelling for the Laser Interferometer Space Antenna","ref_index":94,"is_internal_anchor":false},{"citing_arxiv_id":"2601.14979","citing_title":"The relativistic restricted three-body problem: geometry and motion around tidally perturbed black holes","ref_index":98,"is_internal_anchor":false},{"citing_arxiv_id":"2604.24413","citing_title":"Gravitational waves of extreme-mass-ratio inspirals in a rotating black hole with Dehnen dark matter halo","ref_index":7,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5SNO5XU2ERSRMQI6N6BYDFBBSY","json":"https://pith.science/pith/5SNO5XU2ERSRMQI6N6BYDFBBSY.json","graph_json":"https://pith.science/api/pith-number/5SNO5XU2ERSRMQI6N6BYDFBBSY/graph.json","events_json":"https://pith.science/api/pith-number/5SNO5XU2ERSRMQI6N6BYDFBBSY/events.json","paper":"https://pith.science/paper/5SNO5XU2"},"agent_actions":{"view_html":"https://pith.science/pith/5SNO5XU2ERSRMQI6N6BYDFBBSY","download_json":"https://pith.science/pith/5SNO5XU2ERSRMQI6N6BYDFBBSY.json","view_paper":"https://pith.science/paper/5SNO5XU2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2205.04808&json=true","fetch_graph":"https://pith.science/api/pith-number/5SNO5XU2ERSRMQI6N6BYDFBBSY/graph.json","fetch_events":"https://pith.science/api/pith-number/5SNO5XU2ERSRMQI6N6BYDFBBSY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5SNO5XU2ERSRMQI6N6BYDFBBSY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5SNO5XU2ERSRMQI6N6BYDFBBSY/action/storage_attestation","attest_author":"https://pith.science/pith/5SNO5XU2ERSRMQI6N6BYDFBBSY/action/author_attestation","sign_citation":"https://pith.science/pith/5SNO5XU2ERSRMQI6N6BYDFBBSY/action/citation_signature","submit_replication":"https://pith.science/pith/5SNO5XU2ERSRMQI6N6BYDFBBSY/action/replication_record"}},"created_at":"2026-07-05T06:11:31.806379+00:00","updated_at":"2026-07-05T06:11:31.806379+00:00"}