{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:BCGMD37QGNUXVWWZKHCSRAF2RW","short_pith_number":"pith:BCGMD37Q","schema_version":"1.0","canonical_sha256":"088cc1eff033697adad951c52880ba8d9ebcd578a1cea943f88de9da409cd149","source":{"kind":"arxiv","id":"2506.14868","version":2},"attestation_state":"computed","paper":{"title":"Gravitational waves from b-EMRIs: Doppler shift and beaming, resonant excitation, helicity oscillations and self-lensing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","physics.class-ph"],"primary_cat":"gr-qc","authors_text":"Jo\\~ao S. Santos, Jos\\'e Nat\\'ario, Maarten van de Meent, Vitor Cardoso","submitted_at":"2025-06-17T18:00:00Z","abstract_excerpt":"We study gravitational waves from a stellar-mass binary orbiting a spinning supermassive black hole, a system referred to as a binary extreme mass ratio inspiral (b-EMRI). We use Dixon's formalism to describe the stellar-mass binary as a particle with internal structure, and keep terms up to quadrupole order to capture the generation of gravitational waves by the inner motion of the stellar-mass binary. The problem of emission and propagation of waves is treated from first principles using black hole perturbation theory. In the gravitational waveform at future null infinity, we identify for th"},"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":"2506.14868","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2025-06-17T18:00:00Z","cross_cats_sorted":["astro-ph.HE","physics.class-ph"],"title_canon_sha256":"275f500ffc717c26b5d0ee46488f5807ca9827d0dc5515b0e94ff4354bc14986","abstract_canon_sha256":"4f241d6ea9e0f8cb4b41bae4d136130e8c834d0508ddad09f600152541ef2ede"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:27:31.098525Z","signature_b64":"bUmZ9WqSvE4Ai2FD28jXPWSeEvb7QwkHEiyQ2gWlmNogaqlPZiq0vClgy30D+NWQhSVwrEl8M1K1ii/xBdaZBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"088cc1eff033697adad951c52880ba8d9ebcd578a1cea943f88de9da409cd149","last_reissued_at":"2026-07-05T11:27:31.098018Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:27:31.098018Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational waves from b-EMRIs: Doppler shift and beaming, resonant excitation, helicity oscillations and self-lensing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","physics.class-ph"],"primary_cat":"gr-qc","authors_text":"Jo\\~ao S. Santos, Jos\\'e Nat\\'ario, Maarten van de Meent, Vitor Cardoso","submitted_at":"2025-06-17T18:00:00Z","abstract_excerpt":"We study gravitational waves from a stellar-mass binary orbiting a spinning supermassive black hole, a system referred to as a binary extreme mass ratio inspiral (b-EMRI). We use Dixon's formalism to describe the stellar-mass binary as a particle with internal structure, and keep terms up to quadrupole order to capture the generation of gravitational waves by the inner motion of the stellar-mass binary. The problem of emission and propagation of waves is treated from first principles using black hole perturbation theory. In the gravitational waveform at future null infinity, we identify for th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.14868","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/2506.14868/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":"2506.14868","created_at":"2026-07-05T11:27:31.098074+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.14868v2","created_at":"2026-07-05T11:27:31.098074+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.14868","created_at":"2026-07-05T11:27:31.098074+00:00"},{"alias_kind":"pith_short_12","alias_value":"BCGMD37QGNUX","created_at":"2026-07-05T11:27:31.098074+00:00"},{"alias_kind":"pith_short_16","alias_value":"BCGMD37QGNUXVWWZ","created_at":"2026-07-05T11:27:31.098074+00:00"},{"alias_kind":"pith_short_8","alias_value":"BCGMD37Q","created_at":"2026-07-05T11:27:31.098074+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":8,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.12784","citing_title":"Constraining Kerr supermassive black hole properties using gravitational waves from inspiraling stellar-mass binary black holes","ref_index":27,"is_internal_anchor":false},{"citing_arxiv_id":"2606.28156","citing_title":"Joint inference of line-of-sight acceleration and orbital eccentricity in neutron-star--black-hole binaries","ref_index":135,"is_internal_anchor":false},{"citing_arxiv_id":"2605.22525","citing_title":"Dynamics of Binary System around a Supermassive Black Hole :Binary Scattering and Eccentric vZLK Oscillations","ref_index":85,"is_internal_anchor":false},{"citing_arxiv_id":"2605.20320","citing_title":"Ringdown and lensing of triple systems","ref_index":74,"is_internal_anchor":false},{"citing_arxiv_id":"2507.04471","citing_title":"A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments","ref_index":57,"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":25,"is_internal_anchor":false},{"citing_arxiv_id":"2605.15160","citing_title":"N-body next-to-leading order gravitational spin-orbit interaction via effective field theory","ref_index":91,"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":21,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BCGMD37QGNUXVWWZKHCSRAF2RW","json":"https://pith.science/pith/BCGMD37QGNUXVWWZKHCSRAF2RW.json","graph_json":"https://pith.science/api/pith-number/BCGMD37QGNUXVWWZKHCSRAF2RW/graph.json","events_json":"https://pith.science/api/pith-number/BCGMD37QGNUXVWWZKHCSRAF2RW/events.json","paper":"https://pith.science/paper/BCGMD37Q"},"agent_actions":{"view_html":"https://pith.science/pith/BCGMD37QGNUXVWWZKHCSRAF2RW","download_json":"https://pith.science/pith/BCGMD37QGNUXVWWZKHCSRAF2RW.json","view_paper":"https://pith.science/paper/BCGMD37Q","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.14868&json=true","fetch_graph":"https://pith.science/api/pith-number/BCGMD37QGNUXVWWZKHCSRAF2RW/graph.json","fetch_events":"https://pith.science/api/pith-number/BCGMD37QGNUXVWWZKHCSRAF2RW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BCGMD37QGNUXVWWZKHCSRAF2RW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BCGMD37QGNUXVWWZKHCSRAF2RW/action/storage_attestation","attest_author":"https://pith.science/pith/BCGMD37QGNUXVWWZKHCSRAF2RW/action/author_attestation","sign_citation":"https://pith.science/pith/BCGMD37QGNUXVWWZKHCSRAF2RW/action/citation_signature","submit_replication":"https://pith.science/pith/BCGMD37QGNUXVWWZKHCSRAF2RW/action/replication_record"}},"created_at":"2026-07-05T11:27:31.098074+00:00","updated_at":"2026-07-05T11:27:31.098074+00:00"}