کوروش نوذری

Quantum gravitational effects may affect the large scale dynamics of the universe. Phenomenologically, quantum gravitational effect at large distances can be encoded in an extended uncertainty principle that admits a minimalmeasurablemomentum/energy or amaximal length. This maximal length can be considered as the size of the cosmological horizon today. In this paper we study thermostatistics of an expanding universe as a gaseous system and in the presence of an invariant infrared cutoff.We also compare the thermostatistics of different eras of the evolution of the universe in two classes, Fermions and Bosons.