  We investigate the universe evolution from inflation to late-time
acceleration in a unified way, using a two-component fluid constituted from
extended Chaplygin gas alongside a phantom scalar field. We extract solutions
for the various cosmological eras, focusing on the behavior of the scale
factor, the various density parameters and the equation-of-state parameter.
Furthermore, we extract and discuss bouncing solutions. Finally, we examine the
perturbations of the model, ensuring about their stability and extracting the
predictions for the tensor-to-scalar ratio.
