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Lagrangian and Hamiltonian formulations of asymmetric rigid body, considered as a constrained system
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This work is devoted to a systematic exposition of the dynamics of a rigid body, considered as a system with kinematic constraints. Having accepted the variational problem in accordance with this, we no longer need any additional postulates or assumptions about the behavior of the rigid body. All the basic quantities and characteristics of a rigid body, as well as the equations of motion and integrals of motion, are obtained from the variational problem by direct and unequivocal calculations within the framework of standard methods of classical mechanics. Several equivalent forms for the equations of motion of rotational degrees of freedom are deduced and discussed on this basis. Using the resulting formulation, we revise some cases of integrability, and discuss a number of peculiar properties, that are not always taken into account when formulating the laws of motion of a rigid body.
Forward citations
Cited by 2 Pith papers
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Proposes Poincaré-covariant equations of motion for a discrete relativistic body with six dynamical degrees of freedom, allowing more general motions than Born's theory.
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