{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:I2DBEV3TBFW2667LLDMN5NBJGC","short_pith_number":"pith:I2DBEV3T","schema_version":"1.0","canonical_sha256":"4686125773096daf7beb58d8deb42930aa6c240b60bea68b16ff0e4cad861d2d","source":{"kind":"arxiv","id":"2412.08711","version":1},"attestation_state":"computed","paper":{"title":"New Horizons for Psi: Extreme-Mass-Ratio Inspirals in Fundamental Fields","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Francisco Duque","submitted_at":"2024-12-11T19:00:01Z","abstract_excerpt":"This set of notes guided a 2 hour lecture on \"Extreme-Mass-Ratio Inspirals in Fundamental Fields for the New Horizons for Psi School and Workshop\", hosted at Instituto Superior Tecnico, University of Lisbon, between 1 - 5 July 2024. It introduces how to model asymmetric mass-ratio binaries evolving while immersed in an environment constituted by an ultralight (complex) scalar field using techniques of black hole perturbation theory, and focusing on the simpler example of a spherically symmetric cloud around a non-rotating black hole. A Mathematica notebook with the derivation and solver of the"},"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":"2412.08711","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2024-12-11T19:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"c9e6b93f52974b5ca0e3cf47ece2665de8755f38f7453048145295f1937fd6d1","abstract_canon_sha256":"5066133f69c4c07bd2f83fafe996ec9be560671b2f5f0be795182a66e9f3e7c9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:47:59.344281Z","signature_b64":"25uVmFH9ye/Lt0hpm5di7i2fn194Yxro/V/A96bnQ8RHGqRwD3bUeuY6wI6UuQM3QOuiUN2ojlB6s3Xp+CkJBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4686125773096daf7beb58d8deb42930aa6c240b60bea68b16ff0e4cad861d2d","last_reissued_at":"2026-07-05T09:47:59.343830Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:47:59.343830Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"New Horizons for Psi: Extreme-Mass-Ratio Inspirals in Fundamental Fields","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Francisco Duque","submitted_at":"2024-12-11T19:00:01Z","abstract_excerpt":"This set of notes guided a 2 hour lecture on \"Extreme-Mass-Ratio Inspirals in Fundamental Fields for the New Horizons for Psi School and Workshop\", hosted at Instituto Superior Tecnico, University of Lisbon, between 1 - 5 July 2024. It introduces how to model asymmetric mass-ratio binaries evolving while immersed in an environment constituted by an ultralight (complex) scalar field using techniques of black hole perturbation theory, and focusing on the simpler example of a spherically symmetric cloud around a non-rotating black hole. A Mathematica notebook with the derivation and solver of the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.08711","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/2412.08711/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":"2412.08711","created_at":"2026-07-05T09:47:59.343891+00:00"},{"alias_kind":"arxiv_version","alias_value":"2412.08711v1","created_at":"2026-07-05T09:47:59.343891+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2412.08711","created_at":"2026-07-05T09:47:59.343891+00:00"},{"alias_kind":"pith_short_12","alias_value":"I2DBEV3TBFW2","created_at":"2026-07-05T09:47:59.343891+00:00"},{"alias_kind":"pith_short_16","alias_value":"I2DBEV3TBFW2667L","created_at":"2026-07-05T09:47:59.343891+00:00"},{"alias_kind":"pith_short_8","alias_value":"I2DBEV3T","created_at":"2026-07-05T09:47:59.343891+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2509.08875","citing_title":"Systematic errors in fast relativistic waveforms for Extreme Mass Ratio Inspirals","ref_index":43,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18936","citing_title":"Fine-Tuning Small Reasoning Models for Quantum Field Theory","ref_index":176,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/I2DBEV3TBFW2667LLDMN5NBJGC","json":"https://pith.science/pith/I2DBEV3TBFW2667LLDMN5NBJGC.json","graph_json":"https://pith.science/api/pith-number/I2DBEV3TBFW2667LLDMN5NBJGC/graph.json","events_json":"https://pith.science/api/pith-number/I2DBEV3TBFW2667LLDMN5NBJGC/events.json","paper":"https://pith.science/paper/I2DBEV3T"},"agent_actions":{"view_html":"https://pith.science/pith/I2DBEV3TBFW2667LLDMN5NBJGC","download_json":"https://pith.science/pith/I2DBEV3TBFW2667LLDMN5NBJGC.json","view_paper":"https://pith.science/paper/I2DBEV3T","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2412.08711&json=true","fetch_graph":"https://pith.science/api/pith-number/I2DBEV3TBFW2667LLDMN5NBJGC/graph.json","fetch_events":"https://pith.science/api/pith-number/I2DBEV3TBFW2667LLDMN5NBJGC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I2DBEV3TBFW2667LLDMN5NBJGC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I2DBEV3TBFW2667LLDMN5NBJGC/action/storage_attestation","attest_author":"https://pith.science/pith/I2DBEV3TBFW2667LLDMN5NBJGC/action/author_attestation","sign_citation":"https://pith.science/pith/I2DBEV3TBFW2667LLDMN5NBJGC/action/citation_signature","submit_replication":"https://pith.science/pith/I2DBEV3TBFW2667LLDMN5NBJGC/action/replication_record"}},"created_at":"2026-07-05T09:47:59.343891+00:00","updated_at":"2026-07-05T09:47:59.343891+00:00"}