Pair Instability Supernovae of Very Massive Population III Stars

@article{Chen2014PairIS,
  title={Pair Instability Supernovae of Very Massive Population III Stars},
  author={Ke-Jung Chen and Alexander Heger and S. E. Woosley and Ann S. Almgren and Daniel Whalen Ucsc and UMinn and Monash and Lbnl and Lanl and Ita},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2014}
}
Numerical studies of primordial star formation suggest that the first stars in the universe may have been very massive. Stellar models indicate that non-rotating Population III stars with initial masses of 140-260 Msun die as highly energetic pair-instability supernovae. We present new two-dimensional simulations of primordial pair-instability supernovae done with the CASTRO code. Our simulations begin at earlier times than previous multidimensional models, at the onset of core collapse, to… 
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Finding the First Cosmic Explosions. IV. 90 - 140 M ☉ Pair-instability Supernovae
Population III stars that die as pair-instability supernovae are usually thought to fall in the mass range of 140 - 260 M⊙. However, several lines of work have now shown that rotation can build up
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