No, Einstein's field equations, which form the basis of general relativity, do not change the fact that massive objects attract each other. In fact, one of the major successes of general relativity is that it reproduces Newton's law of universal gravitation in the appropriate limit.
In Newtonian gravity, two massive objects exert a gravitational force on each other that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them. This attractive force causes objects to accelerate towards each other.
Einstein's field equations provide a more comprehensive description of gravity by incorporating the curvature of spacetime. According to general relativity, massive objects curve the fabric of spacetime around them, and the motion of other objects is influenced by this curvature. The field equations relate the distribution of matter and energy to the geometry of spacetime.
When the masses involved and the speeds are small compared to the speed of light, the predictions of general relativity closely resemble Newtonian gravity. In the weak gravitational field limit, the field equations reduce to the Newtonian gravitational law.
However, general relativity goes beyond Newtonian gravity in several important aspects. It accounts for phenomena such as gravitational time dilation, gravitational waves, the bending of light around massive objects, and the expansion of the universe. It provides a more accurate description of gravity in extreme conditions, such as around black holes or during the early stages of the universe.
So, while Einstein's field equations expand our understanding of gravity, they do not negate the basic observation that massive objects attract each other, as described by Newton's law of universal gravitation. Instead, general relativity provides a more comprehensive and accurate framework for describing gravitational phenomena.