The
rotation effect is occasionally disregarded while studying rotating fluid
systems in astronomy, such as stars or gas giant planets. This is due to the
fact that the many stars in our universe revolve around themselves at
comparatively moderate speeds. However, the rotational speed of the fluid
contained in the star's core may reach exceptionally high values when
characterising the internal structure of an astrophysical object. Centrifugal
forces cannot, therefore, be neglected in the fluid motion equation. In this
study, we present a simplified yet comprehensive analysis of rapidly spinning
fluid systems. Then, Euler's equation incorporates the centrifugal force. The
distinctive characteristic of this type of system is revealed by the equation's
solution: "the catastrophe of rapidly spinning fluids." You'll then
observe that the scenario where the fluid is rotating quickly is the one that
most accurately depicts the dynamics in star cores. The nuclear engineer will
employ this novel trait of fluids rotating quickly to build a new style of
nuclear fusion reactor.
Author(s) Details:
Elie W'ishe Sorongane,
Physics Department, University of Kinshasa, Kinshasa, Democratic Republic of the Congo.
Please see the link here: https://stm.bookpi.org/NTPSR-V6/article/view/7214
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