A Dark Energy Quintessence Model of the Universe
Abstract
In this paper, we have presented a model of the FLRW universe filled with matter and dark energy fluids, by assuming an ansatz that deceleration parameter is a linear function of the Hubble constant. This results in a time-dependent DP having decelerating-accelerating transition phase of the universe. This is a quintessence model ω(de)≥ -1. The quintessence phase remains for the period (0 ≤ z ≤ 0.5806). The model is shown to satisfy current observational constraints. Various cosmological parameters relating to the history of the universe have been investigated.
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