Production of the light r-process nuclei in neutrino-driven winds

Details Production of the light r-process nuclei in neutrino-driven winds Production of the light r-process nuclei in neutrino-driven winds

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005nupha.758..667t&link_type=abstract

Nuclear Physics A, Volume 758, p. 667-670.

Physics

Nuclear Physics

Scientific paper

We examine the nucleosynthesis of light r-process nuclei in the neutrino-driven winds from the nascent neutron star resulting from a core-collapse supernova. Neutrino-driven winds are considered to provide most plausible environments for r-process, although requisite conditions for forming the third peak (A=195), which include large neutron excess, high entropy, or short dynamical timescale, cannot be easily obtained. We find that a reasonable fit to the solar r-process abundance distribution in the mass range 90

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