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The dynamics of a flat Friedmann–Robertson–Walker (FRW) cosmological model with a barotropic matter is studied, which is dominated by an oscillating scalar field conformally coupled to the gravity with a scalar potential characterised by multiple vacua. Several motivating consequences are observed and discussed accordingly.

Non-Minimally Conformally Coupling Cosmology with Multiple Vacua Potential with Cubic-Quintic-Septic Duffing Oscillator Properties