Abstract
In classical mechanics Gauss' Theorem for a gravitational field states that, if S is a closed surface and N the component of gravitational force along the outward normal, thenwhere β is the Newtonian constant of gravitation and M is the total mass inside S. This result has recently been extended to general relativity by E. T. Whittaker,1 who, however, considered only the case of a statical gravitational field, the line-element of which is given by2where the coefficients U and αμν are independent of t. It is not immediately clear from his work whether the results are extensible to more general space-times.

This publication has 1 reference indexed in Scilit: