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- W2034118477 abstract "We have studied finite temperature corrections to the baryon transport cross sections and diffusion coefficients. These corrections are based upon our recently computed renormalized electron mass and modified state density due to the background thermal bath in the early universe. It is found that the optimum nucleosynthesis yields computed using our diffusion coefficients shift to longer distance scales by a factor of about 3. We also find that the primordial {sup 4}He abundance decreases by {Delta}Y{sub p}{approx_equal}0.01 while {ital D} and {sup 7}Li increase. The effects of these results on constraints from primordial nucleosynthesis are discussed. In particular, we find that a large baryonic contribution to the closure density ({Omega}{sub b}h{sub 50}{sup 2}{approx_lt}0.4) may be allowed in inhomogeneous models corrected for finite temperature. {copyright} {ital 1998} {ital The American Physical Society}" @default.
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- W2034118477 date "1998-11-16" @default.
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- W2034118477 title "Finite temperature effects on cosmological baryon diffusion and inhomogeneous big-bang nucleosynthesis" @default.
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- W2034118477 doi "https://doi.org/10.1103/physrevd.58.123002" @default.
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