Three-mode Cepheid pulsation. I - The amplitude equations of nonresonant coupling case

Details Three-mode Cepheid pulsation. I - The amplitude equations of nonresonant coupling case Three-mode Cepheid pulsation. I - The amplitude equations of nonresonant coupling case

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.168..243i&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 168, no. 2, June 1990, p. 243-252.

Statistics

Computation

5

Cepheid Variables, Coupled Modes, Stellar Oscillations, Chaos, Computational Astrophysics, Dwarf Stars, Vibration Mode

Scientific paper

Amplitude equations, that are used in the investigation of stellar pulsations, for the three-mode nonresonant coupling case are inferred from that of the two-mode nonresonant coupling case. Characteristics of the fixed points of the amplitude equations are studied. Chaotic behavior is expected when the amplitude equations consists of more than two modes.

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