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Theoretical modeling reveals non-singular cosmic evolution under modified Chaplygin gas dynamics, indicating viable cosmology without modifying general relativity.
The modified Chaplygin gas (MCG) model is revisited to examine its capability in describing the complete cosmic evolution within a unified framework. The model is found to be consistent with observational constraints, including the cosmic microwave background (CMB) shift parameter, while also supporting standard structure formation alongside late-time cosmic acceleration. Due to the highly nonlinear nature of the governing field equations, exact analytical solutions in cosmic time are generally not attainable. To overcome this, we adopt a first-order approximation, which enables us to obtain an analytical expression for the scale factor and determine the corresponding flip time. The effective equation-of-state parameter evolves from a positive value in the early matter-dominated era to weff ≈ -1 w eff ≈ - 1 at late times, in agreement with observations. In addition, a solution in the phantom regime exhibits an emergent, non-singular behavior, where the universe originates from a finite minimum scale factor and smoothly evolves toward a late-time de Sitter-like phase, approaching the Λ Λ CDM limit. The emergent solution is shown to be geodesically complete and free from curvature singularities, as confirmed by the regular behavior of the Kretschmann scalar. We also perform a CMB analysis for all the considered cases, and in each case the obtained values of Rₜₕ R th and χ ²CMB χ CMB 2 remain consistent with observations within the 1σ 1 σ confidence level. Furthermore, the combined Hubble-57 and CMB analysis leads to significantly improved constraints on the model parameters. Moreover, the obtained solutions are independently verified using the Raychaudhuri equation, providing a consistency check that further reinforces the robustness of the methodology. Overall, the results demonstrate that the MCG model provides a self-consistent and observationally viable description of cosmic evolution without requiring modifications to general relativity.
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