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There is one common point on which each astrophysicist believe strongly that most of the contained of our universe is dark and non baryonic. In cultivating recent results it is believe that promising candidates by whom the dark matter is made up are Weakly Interacting Massive Particles (supersymmetric candidate Neutralino) and Axions. A new model is proposed in which Planckian Interacting Massive Particles (PIDMs) are proposed to be the promising dark matter candidates [1]. In this paper we are analyzing the PIDMs with WIMPs to get relic abundance by both of models. Keyword: Dark Matter, Gravitational Interaction

Relic Abundance Analysis by Planckian Interacting Massive Particles and Weakly Interacting Massive Particles