  In this work, we investigate black hole (BH) physics in the context of
gravity rainbow. We investigate this through rainbow functions that have been
proposed by Amelino-Camelia, et el. in [arXiv:0806.0339, hep-th/9605211]. This
modification will give corrections to both the temperature and the entropy of
BH and hence it changes the picture of Hawking radiation greatly when the size
of BH approaches the Planck scale. It prevents BH from total evaporation,
predicting the existence of BH remnant which may resolve the catastrophic
behavior of Hawking radiation as the BH mass approaches zero.
