\begin{document}$ \Omega$\end{document} causes the orbits of particles to move inward with respect to that of the Schwarzschild BH case. Then, the optical properties of a KS BH are studied in detail, that is, the BH shadow and gravitational weak lensing. We demonstrate that the size of the BH shadow decreases under the influence of the KS parameter."> Probing Hořava-Lifshitz gravity using particle and photon dynamics in the presence of plasma -
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