= Hadamard–Rybczynski equation
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The Hadamard–Rybczynski equations describe the motion of a fluid in a gravitational field, particularly in the context of fluid dynamics. These equations are important in studying the behavior of inviscid and incompressible fluids, especially when analyzing potential flow around bodies. The Hadamard–Rybczynski equations relate the velocity potential or stream function to the shape of the body and the flow conditions around it.
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