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Massive Computation for Understanding Core-Collapse Supernova Explosions

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 نشر من قبل Christian D. Ott
 تاريخ النشر 2016
  مجال البحث فيزياء
والبحث باللغة English
 تأليف Christian D. Ott




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How do massive stars explode? Progress toward the answer is driven by increases in compute power. Petascale supercomputers are enabling detailed three-dimensional simulations of core-collapse supernovae. These are elucidating the role of fluid instabilities, turbulence, and magnetic field amplification in supernova engines.



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