Constructing an Inflaton Potential by Mimicking Modified Chaplygin Gas
  In this paper, we considered an inflationary model that effectively behaves
as a modified Chaplygin gas in the context of quintessence cosmology. We
reconstructed the inflaton potential bottom-up and using the recent
observational data we fixed the free parameters of the model. We showed that
the modified Chaplygin gas inspired model is suitable for both the early and
the late time acceleration but has shortcomings between the two periods.
