Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-09-18
Phys.Rev.C58:3696-3710,1998
Astronomy and Astrophysics
Astrophysics
20 pages, 17 figures, Submitted to Physical Review C
Scientific paper
10.1103/PhysRevC.58.3696
We explore neutrino capture during r-process nucleosynthesis in neutrino-driven ejecta from nascent neutron stars. We focus on the interplay between charged-current weak interactions and element synthesis, and we delineate the important role of equilibrium nuclear dynamics. During the period of coexistence of free nucleons and light and/or heavy nuclei, electron neutrino capture inhibits the r-process. At all stages, capture on free neutrons has a larger impact than capture on nuclei. However, neutrino capture on heavey nuclei by itself, if it is very strong, is also detrimental to the r-process until large nuclear equilibrium clusters break down and the classical neutron-capture phase of the r-process begins. The sensitivity of the r-process to neutrino irradiation means that neutrino-capture effects can strongly constrain the r-process site, neutrino physics, or both. These results apply also to r-process scenarios other than neutrino-heated winds.
Fuller George M.
McLaughlin Gail C.
Meyer Bradley S.
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