Abstract
This study delves into the intricate relationship between statistical mechanics and the geometric underpinnings of general relativity within the scope of f(R) gravity theories, with a special emphasis on the cosmological constant (\(\Lambda\)) viewed as a transcendental element. We present a novel formulation of \(f_R(R)\) by synergizing the Lagrangian's Laurent series expansion with thermodynamic entropy considerations, thereby integrating \(\Lambda\) into the modified Einstein field equations. The latter sections offer a rigorous examination of the numerical and semi-analytical solutions for \(\Lambda\) under specific metric constraints, illustrating the inherent complexities in obtaining purely analytical solutions but highlighting the promise of numerical methodologies.