The r-process in supernovae with new microscopic mass formulae

Details The r-process in supernovae with new microscopic mass formulae The r-process in supernovae with new microscopic mass formulae

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005nupha.758..671w&link_type=abstract

Nuclear Physics A, Volume 758, p. 671-674.

Physics

Nuclear Physics

1

Scientific paper

We examine the effects of the newly-derived microscopic Hartree-Fock-Bogoliubov (HFB) mass formulae on the r-process nucleosynthesis and analyse to what extent a solar-like r-abundance distribution can be obtained. The r-process calculations with the HFB-2 mass formula are performed, adopting the parametrized model of the prompt explosion from a collapsing O-Ne-Mg core for the physical conditions. The result is compared with those obtained with the HFB-7 and droplet-type mass formulae.

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