  We present interesting aspects of neutron stars (NSs) from the standpoint of
a modified theory of gravity called Ho\v{r}ava-Lifshitz (HL) gravity. A
deviation from general relativity (GR) in HL gravity can change typical
features of the NS structure. In this study, we investigate the NS structure by
deriving the Tolman-Oppenheimer-Volkoff equation in HL gravity. We find that a
NS in HL gravity with a larger radius and heavier mass than a NS in GR remains
stable without collapsing into a black hole.
