arXiv:astro-ph/9907422·v1·Astrophysics
A detailed analysis of the neutron to proton ratio at the onset of primordial nucleosynthesis
S. Esposito🇮🇹 · G. Mangano🇮🇹 · G. Miele🇮🇹 · O. Pisanti🇮🇹
Abstract
We report on the results of a recent evaluation of all percent level corrections to weak rates of processes converting n <-> p, which are crucial for the determination of the 4He mass fraction produced during primordial nucleosynthesis.
Comments: 5 pages, Talk given at the Second Meeting on New Worlds in Astroparticle Physics, September 1998, Faro, Portugal