Abstract
In this paper we show that the equations of the motion of a free test particle in General Relativity, with respect to any physical system of reference, can always have the classical interpretation:Time derivative of momentum =mass ×gravitational field. The result is reached by means of suitable definitions of the different dynamical quantities relative to the chosen system of reference and by means of the systematic use of a differential operation that generalizes the usual absolute differentiation. In the gravitational field there are present three parts: one deriving from a scalar potential, one similar to Coriolis’ apparent field, and one part deriving from a vector potential.
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