  In this paper, we have studied an interacting dark energy model. We have
assumed the gravitational interaction between the matter fields i.e. between
barotropic fluid and the dark energy. The dark energy evolution within the
framework of spatially homogeneous and isotropic Friedmann-Robertson-Walker
space-time. Therefore, we examine the cosmic evolution from the perspective of
interacting scenario by selecting a suitable ansatz for the scale factor
resulting from a parametrization of Hubble parameter. The evolution of the
cosmological parameters are discussed in some details in the considered
interacting scenario by calculating parameters and quantities such as
deceleration parameter, energy density, pressure, equation of state (EoS) etc.
Also, we have performed some cosmological tests and analysis in support of our
obtained interacting model. Finally, we reconstruct the potential of the scalar
field and refute the refined swampland conjecture using the equation of state
of dark energy and the relationship between energy density and pressure with
the scalar field and potential, and then thoroughly describe the findings.
