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The Geneva stellar evolution code

Eggenberger, P. ; Meynet, G. ; Maeder, A. ; Hirschi, R. ; Charbonnel, C. ; Talon, S. ; Ekström, S.

In: Astrophysics and Space Science, 2008, vol. 316, no. 1-4, p. 43-54

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    Titre
    • The Geneva stellar evolution code
    Auteur
    • Eggenberger, P.. Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes, 1290, Sauverny, Switzerland
    • Meynet, G.. Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes, 1290, Sauverny, Switzerland
    • Maeder, A.. Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes, 1290, Sauverny, Switzerland
    • Hirschi, R.. Department of Physics and Astronomy, University of Basel, Klingelbergstr. 82, 4052, Basel, Switzerland
    • Charbonnel, C.. Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes, 1290, Sauverny, Switzerland
    • Talon, S.. Departement de Physique, Université de Montréal, PQ H3C 3J7, Montréal, Canada
    • Ekström, S.. Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes, 1290, Sauverny, Switzerland
    Type de document
    • Postprint
    Langue
    • Inglese
    Publié dans
    • Astrophysics and Space Science, 2008, vol. 316, no. 1-4, p. 43-54. Springer Netherlands
    Autre version électronique
    Identifiant OAI-PMH
    • oai:doc.rero.ch:315485
    Summary
    This paper presents the Geneva stellar evolution code with special emphasis on the modeling of solar-type stars. The basic input physics used in the Geneva code as well as the modeling of atomic diffusion is first discussed. The physical description of rotation is then presented. Finally, the modeling of magnetic instabilities and transport of angular momentum by internal gravity waves is briefly summarized