The Catastrophe of Rapidly Rotating Fluids
نویسندگان
چکیده
In astrophysics, when studying rotating fluid systems (such as stars or gas giant planets), the rotation effect is most often neglected. This explained by fact that various populate our universe revolve around themselves at relatively low speeds. However, trying to describe internal structure of an astrophysical body, speed contained in core star can reach very high values. It, therefore, becomes impossible neglect centrifugal forces equation motion. this work, we carry out a simplified but above all general study rapidly systems. Euler’s then contains force term. The resolution leads solution reveals particular property type system: “the catastrophe fluids”.
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ژورنال
عنوان ژورنال: Open Journal of Applied Sciences
سال: 2022
ISSN: ['2165-3917', '2165-3925']
DOI: https://doi.org/10.4236/ojapps.2022.124032