BBN observations of light nuclei abundances constrain cosmological models with Weylian boundaries via modified Friedmann equations, numerical thermonuclear rate calculations, and MCMC analysis.
Herrera, Warm inflationary model in loop quantum cosmology, Phys
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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.