A Unified Scale Factor for the Cosmic Evolution -Motivated by Brane World Models- (2505.24420v1)
Abstract: This paper introduces a novel cosmological scale factor, $a(t)=e{H(t)} { (1-e{-k(t)t}) }{b(t)}$, as a strong candidate for effectively modeling the universe in a unified and continuous description across all major epochs of cosmic evolution. We provide a detailed analysis, supported by graphical representations of the universe's evolution with smooth transition from the early inflation to the present acceleration expansion, proposing a coherent and comprehensive picture of cosmic history, consistent with current observational constraints. Furthermore, we explore the theoretical foundations of this model within extra-dimensional physics, demonstrating its compatibility with the brane-world paradigm. Through analytical approximations, the model describes a natural transition from a high-energy, brane-dominated early universe to the low-energy regime governed by general relativity, providing a compelling narrative of cosmic evolution across disparate energy scales. Additionally, the explicit presence of quantum statistical corrections to the Hubble parameter of this scale factor, as a prominent feature of the model, offers a phenomenological approach to incorporating quantum statistic into the classical evolution of the universe.
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