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- W1670199827 abstract "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." @default.
- W1670199827 created "2016-06-24" @default.
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- W1670199827 date "2001-01-01" @default.
- W1670199827 modified "2023-09-27" @default.
- W1670199827 title "Collapse-driven supernovae and the r-process with new data of unstable nuclei" @default.
- W1670199827 doi "https://doi.org/10.1063/1.1372781" @default.
- W1670199827 hasPublicationYear "2001" @default.
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