Published Paper Details:

The origin and expansion of the universe remain central questions in cosmology, with gravitational interactions and dark energy playing fundamental roles in shaping cosmic evolution. This paper proposes a hypothetical theoretical framework that integrates gravitational effects and dark energy dynamics to explain the universe's origin and large-scale expansion. By considering the interplay between these forces, we explore potential mechanisms that could have driven the initial conditions of the universe, from the Big Bang to present-day accelerated expansion. The framework hypothesizes a dynamic equilibrium between gravitational attraction and dark energy repulsion, influencing galaxy formation, cosmic structure evolution, and large-scale anisotropies. Additionally, we investigate how variations in dark energy density and gravitational constants over cosmic time could provide insights into unresolved cosmological puzzles, such as dark matter interactions and the fate of the universe. This study aims to offer a new perspective on the fundamental forces governing cosmic evolution and proposes testable predictions that could be explored through future observational and theoretical advancements.