Non-spherical core collapse supernovae and nucleosynthesis

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Non-spherical core collapse supernovae and nucleosynthesis

Motivated by observations of supernova SN1987A, various authors have simulated Rayleigh–Taylor (RT) instabilities in the envelopes of core collapse supernovae (for a review, see [1]). The non-radial motion found in these simulations qualitatively agreed with observations in SN1987A, but failed to explain the extent of mixing of newly synthesized Ni quantitatively. Here we present results of a 2...

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ژورنال

عنوان ژورنال: Nuclear Physics A

سال: 2001

ISSN: 0375-9474

DOI: 10.1016/s0375-9474(01)00691-1