Stability analysis of the solutions of the local mixing-length theory of convection with convective helium flux

Details Stability analysis of the solutions of the local mixing-length theory of convection with convective helium flux Stability analysis of the solutions of the local mixing-length theory of convection with convective helium flux

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994mnras.271...57n&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 271, 57

Astronomy and Astrophysics

Astronomy

6

Scientific paper

A stability analysis of the two solutions of the extended local mixing-length theory (Umezu & Nakakita) has been performed. It is found that the Yi -convection is stable while the y2-convection is unstable with the ordinarily accepted values of parameters. By linear stability analysis, it can be shown that the maximum V in stable convection is smaller than the value previously given by us and hence than the Ledoux-Sakashita-Hayashi criterion. Key words: convection - instabilities - stars: evolution - stars: interiors.

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