Hostname: page-component-77c89778f8-sh8wx Total loading time: 0 Render date: 2024-07-17T12:52:35.185Z Has data issue: false hasContentIssue false
  • English
  • Français

3D and Some Other Things Missing from the Theory of Massive Star Evolution

Published online by Cambridge University Press:  23 January 2015

W. David Arnett
W. David Arnett*
Affiliation:
Steward Observatory, University of Arizona, Tucson AZ 85721, USA email: darnett@as.arizona.edu
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Keywords

convectionturbulenceSun: abundancesstars: evolutionsupernovae
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Issue S307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry , June 2014 , pp. 459 - 469
Copyright
Copyright © International Astronomical Union 2015 

References

Aerts, C., Christensen-Dalsgaard, J., & Kurtz, D. W. 2010, Asteroseismology, SpringerCrossRefGoogle Scholar
Arnett, D., Meakin, C., & Young, P. A. 2009, ApJ 690, 1715CrossRefGoogle Scholar
Arnett, W. D. & Meakin, C. 2011a, ApJ 733, 78CrossRefGoogle Scholar
Arnett, W. D. & Meakin, C. 2011b, ApJ 741, 33CrossRefGoogle Scholar
Arnett, W. D., Meakin, C., & Viallet, M. 2014, AIP Advances 4 (4), 041010CrossRefGoogle Scholar
Asplund, M., Grevesse, N., Sauval, A. J., & Scott, P. 2009, ARA&A 47, 481Google Scholar
Böhm-Vitense, E. 1958, ZfA 46, 108Google Scholar
Brun, A. S. (ed.) 2011, Astrophysical Dynamics: From Stars to Galaxies, Vol. S 271, International Astronomical Union, CUPGoogle Scholar
Brun, A. S., Miesch, M. S., & Toomre, J. 2004, ApJ 614, 1073CrossRefGoogle Scholar
Brun, A. S., Miesch, M. S., & Toomre, J. 2011, ApJ 742, 79CrossRefGoogle Scholar
Couch, S. M. & Ott, C. D. 2013, ApJ (Letters) 778, L7CrossRefGoogle Scholar
Eggleton, P. P. 1973, MNRAS 163, 279CrossRefGoogle Scholar
Grinstein, F. F., Margolin, L. G., & Rider, W. J. (eds.) 2007, Implicit Large Eddy Simulations, Cambridge University PressCrossRefGoogle Scholar
Grolsch, A. 2015, in Proceedings of this conferenceGoogle Scholar
Herwig, F., Woodward, P. R., Lin, P.-H., Knox, M., & Fryer, C. 2013, ArXiv e-printsGoogle Scholar
Hurlburt, N. E., Toomre, J., & Massaguer, J. M. 1984, ApJ 282, 557CrossRefGoogle Scholar
Kochanek, C. S. 2014, MNRASGoogle Scholar
Kolmogorov, A. 1941, Akademiia Nauk SSSR Doklady 30, 301Google Scholar
Kolmogorov, A. N. 1962, Journal of Fluid Mechanics 13, 82CrossRefGoogle Scholar
Landau, L. D. & Lifshitz, E. M. 1959, Fluid mechanics, PergamonGoogle Scholar
Lorenz, E. N. 1963, Journal of Atmospheric Sciences 20, 1302.0.CO;2>CrossRefGoogle Scholar
Maeder, André 1999, Physics, Formation and Evolution of Rotating Stars, SpringerGoogle Scholar
Magic, Z., Collet, R., Asplund, M., et al. 2013, A&A 557, A26Google Scholar
Magic, Z., Weiss, A., & Asplund, M. 2014, ArXiv e-printsGoogle Scholar
Meakin, C. 2015, in Proceedings of this conferenceGoogle Scholar
Meakin, C. A. & Arnett, D. 2007, ApJ 667, 448CrossRefGoogle Scholar
Meakin, C. A. & Arnett, W. D. 2010, Ap&SS 328, 221Google Scholar
Mocák, M., Meakin, C., Viallet, M., & Arnett, D. 2014, ArXiv e-printsGoogle Scholar
Prandtl, L. & Tietjens, O. G. 1934, Applied Hydro-& Aeromechanics, Dover Publications, Inc.Google Scholar
Smith, N. & Arnett, W. D. 2014, ApJ 785, 82CrossRefGoogle Scholar
Stein, R. F. & Nordlund, Å. 1998, ApJ 499, 914CrossRefGoogle Scholar
Viallet, M., Meakin, C., Arnett, D., & Mocák, M. 2013, ApJ 769, 1CrossRefGoogle Scholar
Vitense, E. 1953, ZfA 32, 135Google Scholar
Wood, T. S., Garaud, P., & Stellmach, S. 2013, ApJ 768, 157CrossRefGoogle Scholar