THE TWO-BODY PROBLEM WITHIN 4D SPACETIME
Symmetrical motion of two objects within 4D Euclidean spacetime:
There are two massive objects in the space of E0a and E0b energy (mass); and ra and rb radius; at a mutual distance of l0; that will start to move toward each other due to the effects of gravity (or toward their joint
barycentre).
The total gravitational potential of bodies is “shared” together so the symmetry of motion is preserved
(the Momentum Conservation Principle), within 4D Euclidean spacetime.
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