Authors: Bruno R Galeffi
This study considers the self-division of a preexisting Substance at high entropy as the seeding and nucleation for the cosmic expansion driven by Friedmann equations. The initial split creates two unsymmetrical constituents that provide the potential energy required for activating the universe expansion and the emergence of three other vacuum components. Hence, this model corresponds to a vacuum containing five ingredients, two with positive and three with negative energy densities, including a negative time-dependent cosmological constant Λ(t). A four-parameter Weibull growth function is used to model the evolution of R(t).
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[v1] 2019-09-28 10:44:52
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