2011/05/31 by Zsolt Horváth, László Á. Gergely, Zoltán Keresztes +2 · 1 citation
Physics and Astronomy · #gr-qc #astro-ph.GA #hep-th
paper · pdf · doi:10.1103/physrevd.84.083006
published as Phys.Rev.D84:083006,2011 · 11 pages, 6 figures, introductory part and reference list changed on referee request, results expanded. Published version
arxiv created 2011/10/13 · arxiv updated 2011/10/14
We discuss gravitational lensing in the Kehagias-Sfetsos space-time emerging in the framework of Hořava-Lifshitz gravity. In weak lensing we show that there are three regimes, depending on the value of λ=1/ωd2, where ω is the Hořava-Lifshitz parameter and d characterizes the lensing geometry. When λ is close to zero, light deflection typically produces two images, as in Schwarzschild lensing. For very large λ the space-time approaches flatness, therefore there is only one undeflected image. In the intermediate range of λ only the upper focused image is produced due to the existence of a maximal deflection angle δmax, a feature inexistent in the Schwarzschild weak lensing. We also discuss the location of Einstein rings, and determine the range of the Hořava-Lifshitz parameter compatible with present day lensing observations. Finally, we analyze in the strong lensing regime the first two relativistic Einstein rings and determine the constraints on the parameter range to be imposed by forthcoming experiments.