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- W62433583 abstract "The simultaneous evolution of weak and nuclear reactions along with baryon diffusion in isothermal fluctuations produced in the quark-hadron phase transition is discussed. We find that the resulting light-element nucleosynthesis is sensitive to the separation distance between fluctuations, although still consistent with observed light-element abundances (except possibly /sup 7/Li) for a reasonable range of separations between fluctuations. The heavy-element nucleosynthesis has been computed for all nuclei up to A = 28. It appears that an r-process ''seed'' abundance will be formed with a mass fraction of 10/sup /minus/12/ to 10/sup /minus/10/. It is not yet clear whether this will lead to an overproduction of r-process abundances relative to that observed in metal-poor halo stars. The evolution of the fluctuations after nucleosynthesis is discussed and it is concluded that these fluctuations are not likely to collapse to form compact cold-dark-matter remnants, but are probably smoothed by baryon diffusion before recombination. 17 refs., 3 figs." @default.
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- W62433583 date "1988-06-01" @default.
- W62433583 modified "2023-09-27" @default.
- W62433583 title "The evolution of baryon number density fluctuations before, during and after primordial nucleosynthesis" @default.
- W62433583 hasPublicationYear "1988" @default.
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