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- W3100687170 abstract "We investigate the nucleosynthesis in the neutrino-driven winds blown off from a $3M_odot$ massive proto-neutron star (mPNS) temporarily formed during the collapse of a $100M_odot$ star. Such mPNSs would be formed in hypernovae. We construct steady and spherically symmetric wind solutions. We set large neutrino luminosities of $sim 10^{53} {rm erg s^{-1}}$ and average energies of electron neutrinos and antineutrinos in the ranges of $epsilon_{nu_e}=9-16 {rm MeV}$ and $epsilon_{bar{nu}_e}=11-18 {rm MeV}$ based on a recent numerical relativity simulation. The wind solutions indicate much shorter temperature-decrease timescale than that of the winds from ordinary PNSs and, depending on $epsilon_nu$, the winds can be both neutron-rich and proton-rich. In the neutron-rich wind, the $r$-process occurs and the abundance distribution of a fiducial wind model of the mPNS gives an approximate agreement with the abundance pattern of metal-poor weak $r$ star HD~122563, although the third-peak elements are produced only when the $bar{nu}_e$ energy is much larger than the $nu_e$ energy. In the proton-rich wind, the strong $nu p$-process occurs and $A>100$ nuclides are synthesized. The synthesized nuclei can be neutron-rich in some cases because the large neutrino luminosity of the mPNS supplies a sufficient amount of neutrons." @default.
- W3100687170 created "2020-11-23" @default.
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- W3100687170 date "2015-09-04" @default.
- W3100687170 modified "2023-10-14" @default.
- W3100687170 title "NUCLEOSYNTHESIS IN NEUTRINO-DRIVEN WINDS IN HYPERNOVAE" @default.
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- W3100687170 doi "https://doi.org/10.1088/0004-637x/810/2/115" @default.
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