Theoretical analysis demonstrates covariant equations of motion for spinning particles in gravitational fields, suggesting improved modeling of relativistic trajectories.
A method for the derivation of the equations of motion of test particles in a given gravitational field is developed. The equations of motion of spinning test particles are derived. The transformation properties are discussed and the equations of motion are written in a covariant form.
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E. Corinaldesi (1951) studied this question.
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