Coupling of thermal and nuclear modes at highly evolved stars

Details Coupling of thermal and nuclear modes at highly evolved stars Coupling of thermal and nuclear modes at highly evolved stars

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..63..237s&link_type=abstract

Astrophysics and Space Science, vol. 63, no. 1, June 1979, p. 237-245.

Computer Science

Numerical Analysis

1

Nuclear Astrophysics, Nuclear Structure, Stellar Evolution, Stellar Models, Abundance, Continuous Spectra, Coupled Modes, Eigenvalues, Numerical Analysis, Secular Variations, Thermal Instability

Scientific paper

An analytical one-zone model (shell source) shows complex secular modes
if perturbations of chemical abundances are included. Very short periods
can be calculated by choosing physically reasonable sets of parameters.
Complex eigenvalues with unstable real parts may be regarded as thermal
instabilities with high-frequency amplitude modulation.

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