{"paper":{"title":"Gravitational radiation from a particle in circular orbit around a black hole. V. Black-hole absorption and tail corrections","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Eric Poisson, Misao Sasaki","submitted_at":"1994-12-08T18:50:20Z","abstract_excerpt":"A particle of mass $\\mu$ moves on a circular orbit of a nonrotating black hole of mass $M$. Under the restrictions $\\mu/M \\ll 1$ and $v \\ll 1$, where $v$ is the orbital velocity, we consider the gravitational waves emitted by such a binary system. We calculate $\\dot{E}$, the rate at which the gravitational waves remove energy from the system. The total energy loss is given by $\\dot{E} = \\dot{E}^\\infty + \\dot{E}^H$, where $\\dot{E}^\\infty$ denotes that part of the gravitational-wave energy which is carried off to infinity, while $\\dot{E}^H$ denotes the part which is absorbed by the black hole. W"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/9412027","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/gr-qc/9412027/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"}