The current value of the scale factor (R₀) is not a fixed number, as it can vary based on the cosmological model being used. In cosmology, R(t) represents the scale factor at time t, and at the current epoch, R(t) equals R₀. The relationship a = R(t)/R₀ indicates that R₀ can be normalized to 1 for convenience in calculations. If the universe is not spatially flat, R₀ can be calculated using specific formulas involving parameters like the Hubble constant and density parameters. Ultimately, R₀ is arbitrary in a flat universe and can be adjusted according to the chosen cosmological framework.