%0 Journal Article
%T Galaxy Rotation Curves in Covariant Ho£żava-Lifshitz Gravity
%A Jean Alexandre
%A Martyna Kostacinska
%J Galaxies
%D 2014
%I MDPI AG
%R 10.3390/galaxies2010001
%X Using the multiplicity of solutions for the projectable case of the covariant extension of Ho£żava-Lifshitz gravity, we show that an appropriate choice for the auxiliary field allows for an effective description of galaxy rotation curves. This description is based on static and spherically symmetric solutions of covariant Ho£żava-Lifshitz gravity and does not require Dark Matter.
%K modified gravity
%K covariant Ho£żava-Lifshitz gravity
%K static and spherically symmetric solution
%K galaxy rotation curves
%U http://www.mdpi.com/2075-4434/2/1/1