Effects of The Dark Energy Hypothesis on the Dynamics of Newtonian Cosmology

Current cosmological theories and simulations by numerous writers are heavily debating the idea of “dark energy,” which is a highly heated issue. This paper aims to understand how dark energy affects the dynamics of the Newtonian Cosmos according to Alagar Ramanujam’s recently proposed cosmological model, The Space Transformation Cosmological Model (STCM 2018), in which the functional aspects of dark energy and the source of the cosmic egg whose expansion produced the current universe have been extensively employed and discussed. The structure of Newtonian Cosmology in the early universe differs significantly from the structure of the rules in the present universe, as demonstrated by this exercise. The scientifically verified inflationary expansion of the early cosmos turns out to be a logical prediction of the theory, which is a key outcome of the exercise described in this study.