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- W3100998930 abstract "The structure of strange dwarfs and that of hybrid stars with the same baryonic number is compared. There is a critical mass (M ≈ 0.24M ⊙ ) in the strange dwarf branch, below which configurations with the same baryonic number in the hybrid star branch are more stable. If a transition occurs between both branches, the collapse releases an energy of about of 3 × 10 50 erg , mostly in the form of neutrinos resulting from the conversion of hadronic matter onto strange quark matter. Only a fraction (~ 4%) is required to expel the outer neutron-rich layers. These events may contribute significantly to the chemical yield of nuclides with A ≥ 80 in the Galaxy, if their frequency is of about one per 1,500 years." @default.
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- W3100998930 date "2006-02-01" @default.
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- W3100998930 title "ARE NEUTRON-RICH ELEMENTS PRODUCED IN THE COLLAPSE OF STRANGE DWARFS?" @default.
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- W3100998930 doi "https://doi.org/10.1142/s0218271806007584" @default.
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