International Journal of Modern Physics D, cilt.33, sa.12, 2024 (SCI-Expanded)
In this paper, we determine the exact solutions of viscous ghost models in sign-changeable interaction scenarios for two choices of bouncing scale factor, assuming the existence of viscous interacting °uid across the °at Friedmann{Robertson{Walker universe in the form of ghost dark energy and pressure-less dark matter. The study demonstrates how the cosmological parameters evolve in viscous sign-changeable interacting scenarios to see the transition time frame. Next, a bounce in°ation model is investigated, including the tensor-to-scalar ratio, scalar spectral index, and slow-roll parameters analytical results. Since in°ation is usually associated with scalar ¯elds, the study looked at a possible relationship between sign-changeable interacting ghost dark °uids and scalar ¯eld models. Lastly, the applicability of the generalized second law (GSL) of thermodynamics is examined for the scenarios that are being studied.