{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:N4NJWNSEMJO66JD53RAIUCFJFN","short_pith_number":"pith:N4NJWNSE","schema_version":"1.0","canonical_sha256":"6f1a9b3644625def247ddc408a08a92b5b08f293bbeb462f651c3474cf2ca04f","source":{"kind":"arxiv","id":"2102.02713","version":5},"attestation_state":"computed","paper":{"title":"Adiabatic waveforms for extreme mass-ratio inspirals via multivoice decomposition in time and frequency","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Alvin J. K. Chua, Gaurav Khanna, Michael L. Katz, Niels Warburton, Scott A. Hughes","submitted_at":"2021-02-04T16:12:22Z","abstract_excerpt":"We compute adiabatic waveforms for extreme mass-ratio inspirals (EMRIs) by \"stitching\" together a long inspiral waveform from a sequence of waveform snapshots, each of which corresponds to a particular geodesic orbit. We show that the complicated total waveform can be regarded as a sum of \"voices.\" Each voice evolves in a simple way on long timescales, a property which can be exploited to efficiently produce waveform models that faithfully encode the properties of EMRI systems. We look at examples for a range of different orbital geometries: spherical orbits, equatorial eccentric orbits, and o"},"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":"2102.02713","kind":"arxiv","version":5},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2021-02-04T16:12:22Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"6759e0f0ad55222723357142be3df7d56448de9ef3967d1309a2c8aca380732f","abstract_canon_sha256":"1fe9edab6bd614d8ba68140aee4cc3297dd87c6837d6a9874fb3171dd7a0bf51"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:01:56.924146Z","signature_b64":"fNtjsEyVX+GPtwLzX0ZWBbLcLJgp3LD7UK36j+b2EPUZprMO66bfb6bZu/d1lNIfL+Vj8dBguWah+DRO8QRbBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6f1a9b3644625def247ddc408a08a92b5b08f293bbeb462f651c3474cf2ca04f","last_reissued_at":"2026-07-05T08:01:56.923674Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:01:56.923674Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Adiabatic waveforms for extreme mass-ratio inspirals via multivoice decomposition in time and frequency","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Alvin J. K. Chua, Gaurav Khanna, Michael L. Katz, Niels Warburton, Scott A. Hughes","submitted_at":"2021-02-04T16:12:22Z","abstract_excerpt":"We compute adiabatic waveforms for extreme mass-ratio inspirals (EMRIs) by \"stitching\" together a long inspiral waveform from a sequence of waveform snapshots, each of which corresponds to a particular geodesic orbit. We show that the complicated total waveform can be regarded as a sum of \"voices.\" Each voice evolves in a simple way on long timescales, a property which can be exploited to efficiently produce waveform models that faithfully encode the properties of EMRI systems. We look at examples for a range of different orbital geometries: spherical orbits, equatorial eccentric orbits, and o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2102.02713","kind":"arxiv","version":5},"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/2102.02713/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":"2102.02713","created_at":"2026-07-05T08:01:56.923739+00:00"},{"alias_kind":"arxiv_version","alias_value":"2102.02713v5","created_at":"2026-07-05T08:01:56.923739+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2102.02713","created_at":"2026-07-05T08:01:56.923739+00:00"},{"alias_kind":"pith_short_12","alias_value":"N4NJWNSEMJO6","created_at":"2026-07-05T08:01:56.923739+00:00"},{"alias_kind":"pith_short_16","alias_value":"N4NJWNSEMJO66JD5","created_at":"2026-07-05T08:01:56.923739+00:00"},{"alias_kind":"pith_short_8","alias_value":"N4NJWNSE","created_at":"2026-07-05T08:01:56.923739+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":15,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.21439","citing_title":"Relativistic effects in extreme-mass-ratio inspirals within scalar clouds: Eccentric and inclined orbits","ref_index":65,"is_internal_anchor":false},{"citing_arxiv_id":"2606.09766","citing_title":"Modified Teukolsky Formalism for Extreme Mass-Ratio Inspirals in Higher-Derivative Gravity","ref_index":91,"is_internal_anchor":false},{"citing_arxiv_id":"2606.02146","citing_title":"Spectral suppression of black hole ringdown tails","ref_index":47,"is_internal_anchor":false},{"citing_arxiv_id":"2606.27429","citing_title":"Massive scalar fields in eccentric regime: Detectability and constraints from LISA observations of extreme mass-ratio inspirals","ref_index":88,"is_internal_anchor":false},{"citing_arxiv_id":"2605.09250","citing_title":"Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework","ref_index":69,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03756","citing_title":"Resonances as signatures of scalar clouds in eccentric extreme-mass-ratio inspirals","ref_index":46,"is_internal_anchor":false},{"citing_arxiv_id":"2606.30594","citing_title":"Efficient Eccentric Effective-One-Body Dynamics via Near-Identity Averaging Transformations","ref_index":153,"is_internal_anchor":false},{"citing_arxiv_id":"2605.28715","citing_title":"Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM","ref_index":201,"is_internal_anchor":false},{"citing_arxiv_id":"2404.14286","citing_title":"Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA","ref_index":196,"is_internal_anchor":false},{"citing_arxiv_id":"2605.13847","citing_title":"Analytical Fluxes from Generic Schwarzschild Geodesics","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2605.13847","citing_title":"Analytical Fluxes from Generic Schwarzschild Geodesics","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2605.09250","citing_title":"Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework","ref_index":69,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03756","citing_title":"Resonances as signatures of scalar clouds in eccentric extreme-mass-ratio inspirals","ref_index":46,"is_internal_anchor":false},{"citing_arxiv_id":"2605.09250","citing_title":"Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework","ref_index":69,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06009","citing_title":"Are Black Holes Fuzzballs? Probing Horizon-Scale Structure with LISA","ref_index":66,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/N4NJWNSEMJO66JD53RAIUCFJFN","json":"https://pith.science/pith/N4NJWNSEMJO66JD53RAIUCFJFN.json","graph_json":"https://pith.science/api/pith-number/N4NJWNSEMJO66JD53RAIUCFJFN/graph.json","events_json":"https://pith.science/api/pith-number/N4NJWNSEMJO66JD53RAIUCFJFN/events.json","paper":"https://pith.science/paper/N4NJWNSE"},"agent_actions":{"view_html":"https://pith.science/pith/N4NJWNSEMJO66JD53RAIUCFJFN","download_json":"https://pith.science/pith/N4NJWNSEMJO66JD53RAIUCFJFN.json","view_paper":"https://pith.science/paper/N4NJWNSE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2102.02713&json=true","fetch_graph":"https://pith.science/api/pith-number/N4NJWNSEMJO66JD53RAIUCFJFN/graph.json","fetch_events":"https://pith.science/api/pith-number/N4NJWNSEMJO66JD53RAIUCFJFN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/N4NJWNSEMJO66JD53RAIUCFJFN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/N4NJWNSEMJO66JD53RAIUCFJFN/action/storage_attestation","attest_author":"https://pith.science/pith/N4NJWNSEMJO66JD53RAIUCFJFN/action/author_attestation","sign_citation":"https://pith.science/pith/N4NJWNSEMJO66JD53RAIUCFJFN/action/citation_signature","submit_replication":"https://pith.science/pith/N4NJWNSEMJO66JD53RAIUCFJFN/action/replication_record"}},"created_at":"2026-07-05T08:01:56.923739+00:00","updated_at":"2026-07-05T08:01:56.923739+00:00"}