We study the quasinormal modes of the massless scalar field of Park black hole in the Ho\v{r}ava gravity using the third order WKB approximation method and found that black hole is stable against these perturbation. We compare and discuss the results with that of Schwarzschild-de Sitter black hole. Thermodynamic properties of Park black hole are investigated and the thermodynamic behavior of upper mass bound is also studied.
., J. S., & et al. (2013). Thermodynamics and quasinormal modes of Park black hole in Hořava gravity. European Physical Journal C, 73. https://doi.org/10.1140/epjc/s10052-013-2613-5 (Original work published 2013)