  We investigate the analytical behavior of many scalar fields working
collectively, where {\phi} i is the ith scalar field. Furthermore, we evaluate
its parameter values by applying certain constraints on our model parameters,
and then compare these values with current observational data from
Observational data of CMB, BAO and H 0 . Through our results, we deeply observe
that in the dark-energy EOS parameter at the Big Rip always finite with the
pressure and dark energy density divergence.
