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In fluid dynamics, the Kirchhoff equations, named after
Gustav Kirchhoff Gustav Robert Kirchhoff (; 12 March 1824 – 17 October 1887) was a German physicist who contributed to the fundamental understanding of electrical circuits, spectroscopy, and the emission of black-body radiation by heated objects. He ...
, describe the motion of a
rigid body In physics, a rigid body (also known as a rigid object) is a solid body in which deformation is zero or so small it can be neglected. The distance between any two given points on a rigid body remains constant in time regardless of external fo ...
in an
ideal fluid In physics, a perfect fluid is a fluid that can be completely characterized by its rest frame mass density \rho_m and ''isotropic'' pressure ''p''. Real fluids are "sticky" and contain (and conduct) heat. Perfect fluids are idealized models in whi ...
. : \begin & = \times \vec \omega + \times \vec v + \vec Q_h + \vec Q, \\ 0pt & = \times \vec \omega + \vec F_h + \vec F, \\ 0ptT & = \left( \vec \omega^T \tilde I \vec \omega + m v^2 \right) \\ 0pt\vec Q_h & =-\int p \vec x \times \hat n \, d\sigma, \\ 0pt\vec F_h & =-\int p \hat n \, d\sigma \end where \vec \omega and \vec v are the angular and linear velocity vectors at the point \vec x, respectively; \tilde I is the moment of inertia tensor, m is the body's mass; \hat n is a unit normal to the surface of the body at the point \vec x; p is a pressure at this point; \vec Q_h and \vec F_h are the hydrodynamic torque and force acting on the body, respectively; \vec Q and \vec F likewise denote all other torques and forces acting on the body. The integration is performed over the fluid-exposed portion of the body's surface. If the body is completely submerged body in an infinitely large volume of irrotational, incompressible, inviscid fluid, that is at rest at infinity, then the vectors \vec Q_h and \vec F_h can be found via explicit integration, and the dynamics of the body is described by the KirchhoffClebsch equations: : = \times \vec \omega + \times \vec v, \quad = \times \vec \omega, : L(\vec \omega, \vec v) = (A \vec \omega,\vec \omega) + (B \vec \omega,\vec v) + (C \vec v,\vec v) + (\vec k,\vec \omega) + (\vec l,\vec v). Their first integrals read : J_0 = \left(, \vec \omega \right) + \left(, \vec v \right) - L, \quad J_1 = \left(,\right), \quad J_2 = \left(,\right) . Further integration produces explicit expressions for position and velocities.


References

* Kirchhoff G. R. ''Vorlesungen ueber Mathematische Physik, Mechanik''. Lecture 19. Leipzig: Teubner. 1877. * Lamb, H., ''Hydrodynamics''. Sixth Edition Cambridge (UK): Cambridge University Press. 1932. Mechanics Classical mechanics Rigid bodies Gustav Kirchhoff {{fluiddynamics-stub