  In recent years, a growing interest on the equilibrium of compact
astrophysical objects like white dwarf and neutron stars has been manifested.
In particular, various modifications due to Planck scale energy effects have
been considered. In this paper we analyze the modification induced by Gravity's
Rainbow on the equilibrium configurations described by the
Tolman-Oppenheimer-Volkoff (TOV) equation. Our purpose is to explore the
possibility that the Rainbow Planck-scale deformation of space-time could
support the existence of different compact stars.
