{ "id": "0905.1523", "version": "v5", "published": "2009-05-11T01:40:21.000Z", "updated": "2009-08-05T14:58:56.000Z", "title": "Towards constraining of the Horava-Lifshitz gravities", "authors": [ "R. A. Konoplya" ], "comment": "10 pages, 5 figures, Latex, new material and references added, the version accepted for publication in Physics Letters B", "journal": "Phys.Lett.B679:499-503,2009", "doi": "10.1016/j.physletb.2009.07.073", "categories": [ "hep-th", "astro-ph.HE", "gr-qc" ], "abstract": "Recently a renormalizable model of gravity has been proposed, which might be a UV completion of General Relativity (GR) or its infra-red modification, probably with a strongly coupled scalar mode. Although the generic vacuum of the theory is anti-de Sitter one, particular limits of the theory allow for the Minkowski vacuum. In this limit (though without consideration of the strongly coupled scalar field) post-Newtonian coefficients of spherically symmetric solutions coincide with those of the General Relativity. Thus the deviations from the convenient GR should be tested beyond the post-Newtonian corrections, that is for a system with strong gravity at astrophysical scales. In this letter we consider potentially observable properties of black holes in the deformed Horava-Lifshitz gravity with Minkowski vacuum: the gravitational lensing and quasinormal modes. We have showed that the bending angle is seemingly smaller in the considered Horava-Lifshitz gravity than in GR. The quasinormal modes of black holes are longer lived and have larger real oscillation frequency in the Horava-Lifshitz gravity than in GR. These corrections should be observable in the near future experiments on lensing and by gravitational antennas, helping to constrain parameters of the Horava-Lifshitz gravity or to discard it.", "revisions": [ { "version": "v5", "updated": "2009-08-05T14:58:56.000Z" } ], "analyses": { "keywords": [ "horava-lifshitz gravity", "black holes", "strongly coupled scalar", "quasinormal modes", "minkowski vacuum" ], "tags": [ "journal article" ], "publication": { "journal": "Physics Letters B", "year": 2009, "month": "Sep", "volume": 679, "number": 5, "pages": 499 }, "note": { "typesetting": "LaTeX", "pages": 10, "language": "en", "license": "arXiv", "status": "editable", "inspire": 819923, "adsabs": "2009PhLB..679..499K" } } }