{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:DPGMGHU5N7NKTO7FIJO3NODJVI","short_pith_number":"pith:DPGMGHU5","schema_version":"1.0","canonical_sha256":"1bccc31e9d6fdaa9bbe5425db6b869aa3af0984027c10f0bc86f60ce552632e5","source":{"kind":"arxiv","id":"2005.11333","version":2},"attestation_state":"computed","paper":{"title":"Evolution of gas disc-embedded intermediate mass ratio inspirals in the LISA band","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A. Derdzinski, A. MacFadyen, D. D'Orazio, P. Duffell, Z. Haiman","submitted_at":"2020-05-22T18:00:14Z","abstract_excerpt":"Among the potential milliHz gravitational wave (GW) sources for the upcoming space-based interferometer LISA are extreme- or intermediate-mass ratio inspirals (EMRI/IMRIs). These events involve the coalescence of supermassive black holes in the mass range $10^5 M_{\\odot} \\lesssim M \\lesssim 10^7 M_{\\odot}$ with companion BHs of much lower masses. A subset of E/IMRIs are expected to occur in the accretion discs of active galactic nuclei (AGN), where torques exerted by the disc can interfere with the inspiral and cause a phase shift in the GW waveform. Here we use a suite of two-dimensional hydr"},"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":"2005.11333","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-05-22T18:00:14Z","cross_cats_sorted":["astro-ph.EP","astro-ph.GA"],"title_canon_sha256":"9dc50d6ec44982d945e72ab005af325624496e4220e9a8656fdc689ff95f7a31","abstract_canon_sha256":"11655762478e36ceeb6c76d06890374b393120ec9d5e678d390f187dc3ad1dce"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:20:54.771509Z","signature_b64":"poMA/68OZbCn/TVMWn2C58FFygjPwxSy8j5u6wptPl+nkRiF0+3T+LgORLyVoP6mJIgvHTbF1a4QwOuNuSlUDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1bccc31e9d6fdaa9bbe5425db6b869aa3af0984027c10f0bc86f60ce552632e5","last_reissued_at":"2026-07-05T02:20:54.770923Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:20:54.770923Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Evolution of gas disc-embedded intermediate mass ratio inspirals in the LISA band","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A. Derdzinski, A. MacFadyen, D. D'Orazio, P. Duffell, Z. Haiman","submitted_at":"2020-05-22T18:00:14Z","abstract_excerpt":"Among the potential milliHz gravitational wave (GW) sources for the upcoming space-based interferometer LISA are extreme- or intermediate-mass ratio inspirals (EMRI/IMRIs). These events involve the coalescence of supermassive black holes in the mass range $10^5 M_{\\odot} \\lesssim M \\lesssim 10^7 M_{\\odot}$ with companion BHs of much lower masses. A subset of E/IMRIs are expected to occur in the accretion discs of active galactic nuclei (AGN), where torques exerted by the disc can interfere with the inspiral and cause a phase shift in the GW waveform. Here we use a suite of two-dimensional hydr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2005.11333","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/2005.11333/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":"2005.11333","created_at":"2026-07-05T02:20:54.770989+00:00"},{"alias_kind":"arxiv_version","alias_value":"2005.11333v2","created_at":"2026-07-05T02:20:54.770989+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2005.11333","created_at":"2026-07-05T02:20:54.770989+00:00"},{"alias_kind":"pith_short_12","alias_value":"DPGMGHU5N7NK","created_at":"2026-07-05T02:20:54.770989+00:00"},{"alias_kind":"pith_short_16","alias_value":"DPGMGHU5N7NKTO7F","created_at":"2026-07-05T02:20:54.770989+00:00"},{"alias_kind":"pith_short_8","alias_value":"DPGMGHU5","created_at":"2026-07-05T02:20:54.770989+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.17765","citing_title":"Effective description of lensed gravitational waves diffracted by stellar fields","ref_index":103,"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":143,"is_internal_anchor":false},{"citing_arxiv_id":"2311.01300","citing_title":"Waveform Modelling for the Laser Interferometer Space Antenna","ref_index":91,"is_internal_anchor":false},{"citing_arxiv_id":"2510.17967","citing_title":"Scalar fields around black hole binaries in LIGO-Virgo-KAGRA","ref_index":7,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11893","citing_title":"Relativistic signatures of scalar dark matter in extreme-mass-ratio inspirals","ref_index":25,"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":18,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DPGMGHU5N7NKTO7FIJO3NODJVI","json":"https://pith.science/pith/DPGMGHU5N7NKTO7FIJO3NODJVI.json","graph_json":"https://pith.science/api/pith-number/DPGMGHU5N7NKTO7FIJO3NODJVI/graph.json","events_json":"https://pith.science/api/pith-number/DPGMGHU5N7NKTO7FIJO3NODJVI/events.json","paper":"https://pith.science/paper/DPGMGHU5"},"agent_actions":{"view_html":"https://pith.science/pith/DPGMGHU5N7NKTO7FIJO3NODJVI","download_json":"https://pith.science/pith/DPGMGHU5N7NKTO7FIJO3NODJVI.json","view_paper":"https://pith.science/paper/DPGMGHU5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2005.11333&json=true","fetch_graph":"https://pith.science/api/pith-number/DPGMGHU5N7NKTO7FIJO3NODJVI/graph.json","fetch_events":"https://pith.science/api/pith-number/DPGMGHU5N7NKTO7FIJO3NODJVI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DPGMGHU5N7NKTO7FIJO3NODJVI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DPGMGHU5N7NKTO7FIJO3NODJVI/action/storage_attestation","attest_author":"https://pith.science/pith/DPGMGHU5N7NKTO7FIJO3NODJVI/action/author_attestation","sign_citation":"https://pith.science/pith/DPGMGHU5N7NKTO7FIJO3NODJVI/action/citation_signature","submit_replication":"https://pith.science/pith/DPGMGHU5N7NKTO7FIJO3NODJVI/action/replication_record"}},"created_at":"2026-07-05T02:20:54.770989+00:00","updated_at":"2026-07-05T02:20:54.770989+00:00"}