The Catastrophe of Rapidly Rotating Fluids: A Recent Study

When investigating rotating fluid systems (such as stars or gas giant planets) in astrophysics, the rotation effect is sometimes overlooked. The fact that the numerous stars in our universe orbit about themselves at relatively slow speeds explains this. When describing the interior structure of an astrophysical entity, however, the speed of rotation of the fluid contained in the star's core might reach extremely high numbers. It is thus impossible to ignore centrifugal forces in the fluid motion equation. We provide a simplified but overarching examination of fast rotating fluid systems in this paper. The centrifugal force is then included in Euler's equation. The solution to this equation exposes a unique feature of this sort of system: "the catastrophe of rapidly rotating fluids." You will then notice that the configuration where the fluid is in rapid rotation is the one that best describes the dynamics in the cores of stars. This new property of rapidly rotating fluids will be used by the nuclear engineer for the construction of a new type of nuclear fusion reactor.