Abstract
The standard model of cosmology is investigated using a time-dependent cosmological constant Λ and Newton gravitational constant G. The total energy content is described by the modified Chaplygin gas equation of state. It is found that the time-dependent constants coupled with the modified Chaplygin gas interpolate between the earlier matter to the later dark-energy dominated phase of the universe. We also achieve a convergence of the parameter ω→−1, almost at the present time. Thus our model fairly alleviates the cosmic-coincidence problem, which demands ω=−1 at the present time.
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Jamil, M., Rahaman, F. & Kalam, M. Cosmic-coincidence problem and variable constants of physics. Eur. Phys. J. C 60, 149–156 (2009). https://doi.org/10.1140/epjc/s10052-009-0865-x
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DOI: https://doi.org/10.1140/epjc/s10052-009-0865-x