... thickness is dr. Thus,dM(R)dr = 4 2®(r). Here, ® is energy density, and by our choice of units, energy is equal to rest mass, so weinterpret m(r) as the total mass of the star enclosed by a sphere ... gik(grk ,s + gks,r - gsr,k) PrPim0dP s d† = 12 (grk ,s + gks,r - gsr,k) PrPkBut the sum of the second and third terms in parentheses is skew-symmetric in r and k,whereas the ... this leads to Newton&apos ;s Law of Gravity.Exercise Set 14 1. Use Ô2˙ = 4 G® and the divergence theorem to deduce Newton&apos ;s law ÔÔÔÔ˙ = GM/r2 fora spherical mass of uniform density...