**The gravitational field equation g(r,t)**

The (n – β) is part of the first term updates the
direction of the field toward the instantaneous position of the mass m, if it
continues to move with constant velocity. This term is connected with the ‘static’
part of the gravitational field of the mass m.

The second term, which is connected with gravitational
radiation by the moving mass m, requires mass acceleration.

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