BBN observations of light nuclei abundances constrain cosmological models with Weylian boundaries via modified Friedmann equations, numerical thermonuclear rate calculations, and MCMC analysis.
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Big Bang Nucleosynthesis constraints on the cosmological evolution in a Universe with a Weylian Boundary
BBN observations of light nuclei abundances constrain cosmological models with Weylian boundaries via modified Friedmann equations, numerical thermonuclear rate calculations, and MCMC analysis.