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Issue EAS Publications Series
Volume 11, 2004
The Future Astronuclear Physics
Page(s) 131 - 140
DOI 10.1051/eas:2004009

The Future Astronuclear Physics
A. Jorissen, S. Goriely, M. Rayet, L. Siess and H. Boffin (eds)
EAS Publications Series, Vol. 11, 2004

DOI: 10.1051/eas:2004009

Novae Modelling Achievements and Challenges

A. Glasner

Racah Institute of Physics, The Hebrew University, Jerusalem, Israel


Abstract
The detailed modelling of thermonuclear runaways in novae is a great challenge. This paper focuses on issues where the coupling between the hydrodynamic and the nuclear aspects is critical. The mixing of heavy elements at the bottom of the accreted envelope is found to be the most significant problem. Other issues related to the modelling of the mixing at the outer parts of the convective zone and to the details of the early light curve are also discussed.



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