3D and some other things missing from the theory of massive Star Evolution

Research output: Contribution to journalArticle

Abstract

This is a sketch of a 321D approximation which is nonlocal, and thus has nonzero fluxes of KE (to be published in more detail elsewhere). We plan to add this as an option to MESA. Inclusion of KE fluxes seems to help resolve the solar abundance problem (Asplund et al. 2009). Smaller cores may ease the explosion problems with core collapse supernova simulations.

Original languageEnglish (US)
Pages (from-to)459-460
Number of pages2
JournalProceedings of the International Astronomical Union
Volume9
DOIs
StatePublished - 2014

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massive stars
explosion
simulation
supernovae
explosions
inclusions
approximation
plan

Keywords

  • convection
  • stars: evolution
  • Sun: abundances
  • supernovae
  • turbulence

ASJC Scopus subject areas

  • Astronomy and Astrophysics

Cite this

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abstract = "This is a sketch of a 321D approximation which is nonlocal, and thus has nonzero fluxes of KE (to be published in more detail elsewhere). We plan to add this as an option to MESA. Inclusion of KE fluxes seems to help resolve the solar abundance problem (Asplund et al. 2009). Smaller cores may ease the explosion problems with core collapse supernova simulations.",
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year = "2014",
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KW - turbulence

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