Collapse-driven supernovae and the r-process with new data of unstable nuclei

Details Collapse-driven supernovae and the r-process with new data of unstable nuclei Collapse-driven supernovae and the r-process with new data of unstable nuclei

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..561...48s&link_type=abstract

TOURS SYMPOSIUM ON NUCLEAR PHYSICS IV: TOURS 2000. AIP Conference Proceedings, Volume 561, pp. 48-52 (2001).

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Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Supernovae, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

We have studied the ν-driven winds from the nascent proto-neutron star. We have found in the general relativistic hydrodynamical simulations using the relativistic EOS table that the short expansion time scale is realized in the cases of massive and compact proto-neutron stars. Having the trajectories of ejecta, we have performed r-process calculations to find that a successful r-process up to A~195 occurs in the ν-driven winds with a short expansion time scale. .

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