{"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"}