http://arxiv.org/abs/1904.10418
In this work, we have considered a model independent approach to study the nature of the late time cosmic acceleration. We have used the Pade approximation to parametrize the comoving distance. Consequently, from this comoving distance, we derive a parameterization for the Hubble parameter. Our parametrization is completely analytic and valid for late-time and matter dominated eras only. This parametrization possesses sub-percentage accuracy compared to any arbitrary cosmological model or parametrization up to matter dominated era. Using this parametrization, we put constraints on the parameters from recent low redshift cosmological observations including Planck 2018 results. Our results show that the $\Lambda$CDM model is 1$\sigma$ away for redshift $z<1.5$. We also find that the dynamical dark energy models are preferred for redshift $z<0.5$.
B. Dinda
Wed, 24 Apr 19
50/51
Comments: 7 pages, 5 figures, and a Table
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