Possible evolution of a bouncing universe in cosmological models with non-minimally coupled scalar fields with bounce solutions evolving on
a spatially flat Friedmann-Lemaître-Robertson-Walker background. We consider
Inflation with a quartic potential in the framework of Einstein-Gauss-Bonnet gravity to the Gauss-Bonnet curvature invariant, so that the latter appears to be dynamically important. We consider
a Possible evolution of a bouncing universe in cosmological models with non-minimally coupled scalar fields with bounce solutions evolving on
a spatially flat Friedmann-Lemaître-Robertson-Walker background. We consider
Cosmological attractor inflation from the RG-improved Higgs sector of finite gauge theory which sums all leading logs of perturbation theory is essential for
a successful realization
Strategies in performing a multi-level C-test: applying Think-Aloud Protocols apply while taking
a multi-level C-test; 2) to examine the correlation between the level of complexity