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Article Dans Une Revue Astronomy and Astrophysics - A&A Année : 2008

Direct numerical simulations of the κ-mechanism. II. Nonlinear saturation and the Hertzsprung progression

Résumé

Context: We study the κ-mechanism that excites radial oscillations in Cepheid variables. Aims: We address the mode couplings that manage the nonlinear saturation of the instability in direct numerical simulations (DNS). Methods: We project the DNS fields onto an acoustic subspace built from the regular and adjoint eigenvectors that are solutions to the linear oscillation equations. Results: We determine the time evolution of both the amplitude and kinetic energy of each mode that propagates in the DNS. More than 98% of the total kinetic energy is contained in two modes that correspond to the linearly-unstable fundamental mode and the linearly-stable second overtone. Because the eigenperiod ratio is close to 1/2, we discover that the nonlinear saturation is due to a 2:1 resonance between these two modes. An interesting application of this result concerns the reproduction of Hertzsprung's progression observed in Bump Cepheids.

Dates et versions

hal-00392428 , version 1 (08-06-2009)

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T. Gastine, B. Dintrans. Direct numerical simulations of the κ-mechanism. II. Nonlinear saturation and the Hertzsprung progression. Astronomy and Astrophysics - A&A, 2008, 490, pp.743-752. ⟨10.1051/0004-6361:200809891⟩. ⟨hal-00392428⟩
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