Scalar-fluid interacting dark energy: Cosmological dynamics beyond the exponential potential

We extend the dynamical systems analysis of scalar-fluid interacting dark energy models performed in C.G. Boehmer et al., Phys. Rev. D 91, 123002 (2015) by considering scalar field potentials beyond the exponential type. The properties and stability of critical points are examined using a combination of linear analysis, computational methods and advanced mathematical techniques, such as center manifold theory. We show that the interesting results obtained with an exponential potential can generally be recovered also for more complicated scalar field potentials. In particular, employing power law and hyperbolic potentials as examples, we find late time accelerated attractors, transitions from dark matter to dark energy domination with specific distinguishing features, and accelerated scaling solutions capable of solving the cosmic coincidence problem.