Bi-metric Universe with Matter
Carlos Maldonado, Fernando Mendez

TL;DR
This paper investigates a bi-metric universe model with matter, analyzing how energy transfer between two causally disconnected patches affects early universe evolution and constrains the model's deformation parameter.
Contribution
It introduces a novel bi-metric universe framework with matter, exploring energy transfer dynamics and constraining the deformation parameter based on nucleosynthesis constraints.
Findings
Energy transfers from one sector to the other during early evolution.
The deformation parameter ppa is constrained by nucleosynthesis temperature.
The model relates to and extends non-standard cosmological theories.
Abstract
We analyze the early stage of evolution of a universe with two scale factors proposed in [1] when matter is present. The scale factors describe two causally disconnected patches of the universe interacting trough a non-trivial Poisson bracket structure in the momentum sector characterized by one parameter \kappa. We studied two scenarios in which one of the patches is always filled with relativistic matter while the other contains relativistic matter in one case, and non-relativistic matter in the second case. By solving numerically the set of equations governing the dynamics, we found that the energy content of one sector drains to the other and from here it is possible to constraint the deformation parameter \kappa by imposing that the decay of the energy density happens, at most, at the Big Bang Nucleosynthesis temperature in order to return to the usual behavior of radiation. The…
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