Study of the reconstructed new holographic dark energy model
Department of Mathematics, University of the Punjab, Quaid-e-Azam Campus, 54590, Lahore, Pakistan
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Accepted: 10 May 2018
Published online: 26 June 2018
In this paper, we explore cosmological consequences of the new holographic dark energy model in the background of gravity. For this purpose, we consider the reconstruction technique as well as the power-law scale factor. We reconstruct the model and investigate its stability by the squared speed of sound parameter. We also discuss the evolution of equation of state, density, deceleration, - plane and statefinder parameters. It is found that reconstructed new holographic dark energy model is stable for a particular range of b, where b is the constant of the power-law scale factor.
© Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature, 2018