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Non-Normal Pulsation

Published online by Cambridge University Press:  15 August 2009

P. Yecko
Affiliation:
Department of Mathematical Sciences, Montclair State University, Montclair, NJ, USA
J. Pohlmeyer
Affiliation:
Department of Mathematical Sciences, Montclair State University, Montclair, NJ, USA
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Abstract

Klein-Gordon operators with complex potentials are formulated as model systems to examine the possible impact of non-normality on the stellar pulsation eigenvalue problem. Computations of spectra, ε-pseudospectra and resolvent norms for these operators show that extended regions of complex potential, corresponding in stars to non-adiabatic regions, leads to strong non-normality. Introduction of an advective term further increases non-normal properties. Prospective model improvements and implications for resonances and for nonlinear pulsation are considered.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2009

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