Nucleosynthesis in the Inhomogeneous Universe and Effects of Neutron Diffusion

Abstract
We investigate nucleosynthesis in the universe with isothermal baryon density fluctuations taking into account nucleon diffusion during the nucleosynthesis. We find Ω B = 1 universe is marginally consistent with the light element abundances (D, 3 He, 4 He, 7 Li) if the density contrast, R is very high, ≳300 and the other parameters are tuned.

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