Researchers have proposed a cosmological model that introduces a bounce mechanism to prevent the universe from reaching a singular state.

The model utilizes a scalar field and dark energy component to maintain a non-singular bounce and turnaround, avoiding issues of diverging scale factor and energy density.

A single positive tension brane approach is used, contrasting with other models and allowing for natural generation of cosmological perturbations.

Future work will involve testing the model against observational data to analyze key parameters.

This innovative approach provides insights into the dynamics of an oscillating universe and the impact of phantom dark energy on its evolution.

The model offers a fresh perspective on cosmological models addressing the initial singularity problem.