Modification of the Exterior and Interior Solution of Einstein’s G22 Field Equation for a Homogeneous Spherical Massive Bodies whose Fields Differ in Radial Size, Polar Angle, and Time.
U. Rilwan1*, A.U. Maisalatee2, E. I. Ugwu1, O. G. Okara3, S. Muhammad1, A. Ubaidullah4 and H. Abdulrahman5 In general theory of relativity, Einstein’s field equations relate the geometry of space-time with the distribution of matter within it. These equations were first published by Einstein in the form of a tensor equation which related the local
















