{"work":{"id":"64d31f4f-7bfb-46ba-bdca-3d761b255c8c","openalex_id":null,"doi":null,"arxiv_id":"hep-th/0611226","raw_key":null,"title":"Gravitational spectrum of black holes in the Einstein-Aether theory","authors":null,"authors_text":"R","year":2006,"venue":"hep-th","abstract":"Evolution of gravitational perturbations, both in time and frequency domains, is considered for a spherically symmetric black hole in the non-reduced Einstein-Aether theory. It is shown that real oscillation frequency and damping rate are larger for the Einstein-Aether black hole than for the Schwarzschild black hole. This may provide an opportunity to observe aether in the forthcoming experiments with new generation of gravitational antennas.","external_url":"https://arxiv.org/abs/hep-th/0611226","cited_by_count":null,"metadata_source":"pith","metadata_fetched_at":"2026-05-16T02:42:10.437379+00:00","pith_arxiv_id":"hep-th/0611226","created_at":"2026-05-10T10:49:56.691486+00:00","updated_at":"2026-05-16T02:42:10.437379+00:00","title_quality_ok":true,"display_title":null,"render_title":"Gravitational spectrum of black holes in the Einstein-Aether theory"},"hub":{"state":{"work_id":"64d31f4f-7bfb-46ba-bdca-3d761b255c8c","tier":"hub","tier_reason":"10+ Pith inbound or 1,000+ external citations","pith_inbound_count":10,"external_cited_by_count":null,"distinct_field_count":1,"first_pith_cited_at":"2026-02-11T16:23:23+00:00","last_pith_cited_at":"2026-05-12T00:34:59+00:00","author_build_status":"not_needed","summary_status":"needed","contexts_status":"needed","graph_status":"needed","ask_index_status":"not_needed","reader_status":"not_needed","recognition_status":"not_needed","updated_at":"2026-05-28T12:28:38.508175+00:00","tier_text":"hub"},"tier":"hub","role_counts":[{"context_role":"background","n":9},{"context_role":"method","n":1}],"polarity_counts":[{"context_polarity":"background","n":8},{"context_polarity":"unclear","n":1},{"context_polarity":"use_method","n":1}],"runs":{},"summary":{},"graph":{},"authors":[]}}