- Kirchhoff equations
The motion of a rigid body in an ideal fluid can be expressed in a basis fixed to the body by Kirchhoff's equations:
where and are the angular and linear velocity vectors at the point , respectively; is the moment of inertia tensor, is the body's mass; isa unit normal to the surface of the body at the point ; is a pressure at this point; and are the hydrodynamictorque and force acting on the body, respectively; and likewise denote all other torques and forces acting on thebody. The integration is performed over the fluid-exposed portion of thebody's surface.
If the body is completely submerged body in an infinitely largevolume of irrotational, incompressible, inviscid fluid, that is atrest at infinity, then the vectors and can befound via explicit integration, and the dynamics of the body isdescribed by the Kirchhoff -
Clebsch equations:Their first integrals read
.
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.
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