{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:3X4G4SATZYACBYXQ6RNKY5N7FK","short_pith_number":"pith:3X4G4SAT","schema_version":"1.0","canonical_sha256":"ddf86e4813ce0020e2f0f45aac75bf2aafa8f8cbeb85e598677fb76324444dbb","source":{"kind":"arxiv","id":"2206.05292","version":2},"attestation_state":"computed","paper":{"title":"The imprint of gas on gravitational waves from LISA intermediate-mass black hole binaries","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE","gr-qc"],"primary_cat":"astro-ph.GA","authors_text":"Andrea Derdzinski, Lorenz Zwick, Lucio Mayer, Mudit Garg, Pedro R. Capelo","submitted_at":"2022-06-10T18:00:00Z","abstract_excerpt":"We study the effect of torques on circular inspirals of intermediate-mass black hole binaries (IMBHBs) embedded in gas discs, wherein both BH masses are in the range $10^2$-$10^5~\\rm{M}_\\odot$, up to redshift $z = 10$. We focus on how torques impact the detected gravitational wave (GW) waveform in the frequency band of the Laser Interferometer Space Antenna (LISA) when the binary separation is within a few hundred Schwarzschild radii. For a sub-Eddington accretion disc with a viscosity coefficient $\\alpha=0.01$, surface density $\\Sigma\\approx10^5$ g cm$^{-2}$, and Mach number $\\mathcal{M}_{\\rm"},"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":"2206.05292","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2022-06-10T18:00:00Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE","gr-qc"],"title_canon_sha256":"6c13849a14f6846553d9a79af766d7f902634410a0cf0112c01d65354bfa9bd6","abstract_canon_sha256":"cf470d66744c25442cb92adbe3b07c5d8869e5365be1ac8eba3631239c59a309"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:04:13.583683Z","signature_b64":"fbwFNIaCU5jLsXL9AmLZ3dgCONGEJVMf+KCdIzeuXan4YbbFVyIRns1t7GmBVLnJdSubF+rx4h8Cwgnttao1Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ddf86e4813ce0020e2f0f45aac75bf2aafa8f8cbeb85e598677fb76324444dbb","last_reissued_at":"2026-07-05T05:04:13.583185Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:04:13.583185Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The imprint of gas on gravitational waves from LISA intermediate-mass black hole binaries","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE","gr-qc"],"primary_cat":"astro-ph.GA","authors_text":"Andrea Derdzinski, Lorenz Zwick, Lucio Mayer, Mudit Garg, Pedro R. Capelo","submitted_at":"2022-06-10T18:00:00Z","abstract_excerpt":"We study the effect of torques on circular inspirals of intermediate-mass black hole binaries (IMBHBs) embedded in gas discs, wherein both BH masses are in the range $10^2$-$10^5~\\rm{M}_\\odot$, up to redshift $z = 10$. We focus on how torques impact the detected gravitational wave (GW) waveform in the frequency band of the Laser Interferometer Space Antenna (LISA) when the binary separation is within a few hundred Schwarzschild radii. For a sub-Eddington accretion disc with a viscosity coefficient $\\alpha=0.01$, surface density $\\Sigma\\approx10^5$ g cm$^{-2}$, and Mach number $\\mathcal{M}_{\\rm"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2206.05292","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/2206.05292/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":"2206.05292","created_at":"2026-07-05T05:04:13.583240+00:00"},{"alias_kind":"arxiv_version","alias_value":"2206.05292v2","created_at":"2026-07-05T05:04:13.583240+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2206.05292","created_at":"2026-07-05T05:04:13.583240+00:00"},{"alias_kind":"pith_short_12","alias_value":"3X4G4SATZYAC","created_at":"2026-07-05T05:04:13.583240+00:00"},{"alias_kind":"pith_short_16","alias_value":"3X4G4SATZYACBYXQ","created_at":"2026-07-05T05:04:13.583240+00:00"},{"alias_kind":"pith_short_8","alias_value":"3X4G4SAT","created_at":"2026-07-05T05:04:13.583240+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2607.00845","citing_title":"Environmental effects vs. modified gravity in the LISA massive black hole binary population","ref_index":39,"is_internal_anchor":false},{"citing_arxiv_id":"2606.27526","citing_title":"Dynamics of Relativistic Binaries in Structured and Stochastic Environments: A Lagrange-Fourier-Hansen Framework","ref_index":99,"is_internal_anchor":false},{"citing_arxiv_id":"2311.01300","citing_title":"Waveform Modelling for the Laser Interferometer Space Antenna","ref_index":65,"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":36,"is_internal_anchor":false},{"citing_arxiv_id":"2509.14924","citing_title":"Residual Test for the Third Gravitational-Wave Transient Catalog","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11893","citing_title":"Relativistic signatures of scalar dark matter in extreme-mass-ratio inspirals","ref_index":27,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3X4G4SATZYACBYXQ6RNKY5N7FK","json":"https://pith.science/pith/3X4G4SATZYACBYXQ6RNKY5N7FK.json","graph_json":"https://pith.science/api/pith-number/3X4G4SATZYACBYXQ6RNKY5N7FK/graph.json","events_json":"https://pith.science/api/pith-number/3X4G4SATZYACBYXQ6RNKY5N7FK/events.json","paper":"https://pith.science/paper/3X4G4SAT"},"agent_actions":{"view_html":"https://pith.science/pith/3X4G4SATZYACBYXQ6RNKY5N7FK","download_json":"https://pith.science/pith/3X4G4SATZYACBYXQ6RNKY5N7FK.json","view_paper":"https://pith.science/paper/3X4G4SAT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2206.05292&json=true","fetch_graph":"https://pith.science/api/pith-number/3X4G4SATZYACBYXQ6RNKY5N7FK/graph.json","fetch_events":"https://pith.science/api/pith-number/3X4G4SATZYACBYXQ6RNKY5N7FK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3X4G4SATZYACBYXQ6RNKY5N7FK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3X4G4SATZYACBYXQ6RNKY5N7FK/action/storage_attestation","attest_author":"https://pith.science/pith/3X4G4SATZYACBYXQ6RNKY5N7FK/action/author_attestation","sign_citation":"https://pith.science/pith/3X4G4SATZYACBYXQ6RNKY5N7FK/action/citation_signature","submit_replication":"https://pith.science/pith/3X4G4SATZYACBYXQ6RNKY5N7FK/action/replication_record"}},"created_at":"2026-07-05T05:04:13.583240+00:00","updated_at":"2026-07-05T05:04:13.583240+00:00"}