Observational Constraints on New Exact Inflationary Scalar-field
  Solutions
  An algorithm is used to generate new solutions of the scalar field equations
in homogeneous and isotropic universes. Solutions can be found for pure scalar
fields with various potentials in the absence and presence of spatial curvature
and other perfect fluids. A series of generalisations of the Chaplygin gas and
bulk viscous cosmological solutions for inflationary universes are found.
Furthermore other closed-form solutions which provide inflationary universes
are presented. We also show how the Hubble slow-roll parameters can be
calculated using the solution algorithm and we compare these inflationary
solutions with the observational data provided by the Planck 2015 collaboration
in order to constraint and rule out some of these models.
