{"paper":{"title":"Linear stability of vector Horndeski black holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Antonio De Felice, Che-Yu Chen, Shinji Tsujikawa","submitted_at":"2024-04-14T23:28:47Z","abstract_excerpt":"Horndeski's vector-tensor (HVT) gravity is described by a Lagrangian in which the field strength $F_{\\mu \\nu}=\\partial_{\\mu} A_{\\nu}-\\partial_{\\nu} A_{\\mu}$ of a vector field $A_{\\mu}$ interacts with a double dual Riemann tensor $L^{\\mu \\nu \\alpha \\beta}$ in the form $\\beta L^{\\mu \\nu \\alpha \\beta} F_{\\mu \\nu} F_{\\alpha \\beta}$, where $\\beta$ is a constant. In Einstein-Maxwell-HVT theory, there are static and spherically symmetric black hole (BH) solutions with electric or magnetic charges, whose metric components are modified from those in the Reissner-Nordstr\\\"om geometry. The electric-magne"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2404.09377","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/2404.09377/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"}