{"paper":{"title":"Condensation for non-relativistic matter in Ho\\v{r}ava-Lifshitz gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Jiliang Jing, Qiyuan Pan, Songbai Chen","submitted_at":"2014-10-29T00:53:37Z","abstract_excerpt":"We study condensation for non-relativistic matter in a Ho\\v{r}ava-Lifshitz black hole without the condition of the detailed balance. We show that, for the fixed non-relativistic parameter $\\alpha_2$ (or the detailed balance parameter $\\epsilon$), it is easier for the scalar hair to form as the parameter $\\epsilon$ (or $\\alpha_2$) becomes larger, but the condensation is not affected by the non-relativistic parameter $\\beta_2$. We also find that the ratio of the gap frequency in conductivity to the critical temperature decreases with the increase of $\\epsilon$ and $\\alpha_2$, but increases with "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.7847","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":""},"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"}