Stellar Evolution and Seismic Tools for Asteroseismology - Diffusive Processes in Stars and Seismic Analysis
C.W. Straka, Y. Lebreton and M.J.P.F.G. Monteiro (eds)
EAS Publications Series, 26 (2007) 79-89
DOI: 10.1051/eas:2007127
The Treatment of Overshooting in Stellar Modelling: Instantaneous and Diffusive Approach
P. VenturaINAF - Osservatorio Astronomico di Roma, via Frascati 33, 00040 MontePorzio Catone (RM), Italy
(Published online: 20 June 2007)
Abstract
Convective overshoot is a physical mechanism for which no recipe
based on first principles is available; hence the necessity of
assuming some parametrisations, which undermine the
predictive power of the current generation of stellar models.
We evidentiate the non local aspects of the convective phenomenon
particularly in the proximities of the convective borders, and
identify some cases when the use of a diffusive rather than the
classic instantaneous approach to describe overshooting is highly
recommended.
© EAS, EDP Sciences 2007


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