BBN deuterium abundances exclude baryon-to-photon inhomogeneities above roughly 26-28% RMS, probing physics at temperatures up to a few TeV.
Nucleosynthesis Without a Computer
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I derive completely analytically the time evolution and final abundances of the light elements (up to Be-7) formed in the big-bang nucleosynthesis.This highlights an interesting physics taking place during the formation of light elements in the early universe.
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The Bearable Inhomogeneity of the Baryon Asymmetry
BBN deuterium abundances exclude baryon-to-photon inhomogeneities above roughly 26-28% RMS, probing physics at temperatures up to a few TeV.