How the nonlinear coupled oscillators modelization explains the Blazhko effect, the synchronisation of layers, the mode selection, the limit cycle, and the red limit of the instability strip
Cyrus Zalian

TL;DR
This paper models RR Lyrae stars as coupled nonlinear oscillators to explain the Blazhko effect, mode selection, layer synchronization, and the red limit of the instability strip, offering a new theoretical framework.
Contribution
It introduces a novel discrete oscillator model that explains multiple phenomena in pulsating stars, including the Blazhko effect, through synchronization and energy transfer mechanisms.
Findings
Explains the Blazhko effect via energy transfer between modes.
Provides a new explanation for the red limit of the instability strip.
Describes mode selection and layer synchronization through coupled oscillators.
Abstract
Context. The Blazhko effect, in RR Lyrae type stars, is a century old mystery. Dozens of theory exists, but none have been able to entirely reproduce the observational facts associated to this modulation phenomenon. Existing theory all rely on the usual continuous modelization of the star. Aims. We present a new paradigm which will not only explain the Blazhko effect, but at the same time, will give us alternative explanations to the red limit of the instability strip, the synchronization of layers, the mode selection and the existence of a limit cycle for radially pulsating stars. Methods. We describe the RR Lyrae type pulsating stars as a system of coupled nonlinear oscillators. Considering a spatial discretisation of the star, supposing a spherical symmetry, we develop the equation of motion and energy up to the third order in the radial and adiabatic case. Then, we include the…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astro and Planetary Science · Geophysics and Sensor Technology
