Abstract
According to the principle of emergence, the expansion of the Universe can be explained as the emergence of space with the progress of cosmic time. We have analytically solved the equation of emergence proposed by Padmanabhan by assuming the Komar energy density ρ + 3P as a function of the Hubble parameter. The resulting model describes the evolution of the Universe, which proceeds towards a final de Sitter state. Model parameters have been extracted using the cosmological observational data. Further, the horizon entropy evolution of the model has been studied. The model predicts a Universe having a transition from a prior decelerated epoch to a late accelerated epoch and reasonably predicts the cosmological constant.
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