In 1975 , the discovery of the Black holes’ temperature and entropy by Hawking , made this field , one of the interesting areas of research . Recently , Verlinde have given a very innovative suggestion considering the origin of the gravitation . He argues that the gravitational force may be described by the entropic force . Based on holographic principle , he assumed the information storage on the holographic surfaces . This principle postulate that the maximum amount of information stored on the space is proportional to all N bits on the holographic surfaces . In this dissertation , we explore a system of gas that includes N bosonic particles in the near horizon region . Following the above ideas , we demonstrated that in the condensed state , the Hawking temperature is exactly the temperature in which the transition occur . Our method also yields the entropy of black holes and confirms the result that it is proportional to the event horizon area . In this thesis we are concerned with the effect of the Generalized Uncertainty Principle (GUP) on the black holes’ entropy , the corrections to the Hawking’s temperature , the phase transition temperature and the other thermodynamics variables , which are investigated in the last section .