On a simple model for describing convection of the rotating fluid: integrability, bifurcations and global dynamics

TL;DR

This paper analyzes the Glukhovsky-Dolzhansky model for rotating fluid convection, revealing its integrability properties, bifurcations, global attractors, and complex dynamics at infinity, with implications for geophysical fluid studies.

Contribution

It provides a complete classification of Darboux polynomials, identifies integrable cases, and studies the global dynamics and bifurcations of the GD model.

Findings

GD model has no polynomial, rational, or Darboux first integrals.

Existence of a global attractor is proved.

The model exhibits two dynamical transitions as Rayleigh number increases.

Abstract

The Glukhovsky-Dolzhansky (GD) model arises naturally from geophysical science, which describes rotating fluid convection inside the ellipsoid. This work aims to provide some new insights into the GD model. (\emph{i}) We first show that, under some conditions there are homothetic transformations which covert the GD model into other similar quadric physical models, therefore, our results on the GD model can be naturally applied to the investigation of these models. (\emph{ii}) We propose a complete classification of Darboux polynomials and exponent factors for the GD model, which implies that the GD model has no polynomial, rational, or Darboux first integrals. In addition, some integrable cases of the GD model are also given when the physical parameters are allowed to be non-positive. (\emph{iii}) The existence of global attractor is proved. The stability and local bifurcations of all co-dimension one and two are investigated. Particularly, we show that the GD model undergoes two dynamical transitions as the Rayleigh number increases. (\emph{iv}) To understand the asymptotic behavior of the orbits for the GD model, we use the Poincar\'{e} compactification method to study its dynamical behavior at infinity. More precisely, we prove that the phase portraits of the GD model at infinity consist of an infinite sequence of periodic solutions and two heteroclinic loops. Our results may help us better understand the complex and rich dynamics of rotating fluid convection.