Post-Newtonian expansions in
general relativity are used for finding an approximate solution of the
Einstein field equations for the
metric tensor. The approximations are expanded in small parameters which express orders of deviations from
Newton's law of universal gravitation. This allows approximations to Einstein's equations to be made in the case of weak fields. Higher order terms can be added to increase accuracy, but for strong fields sometimes it is preferable to solve the complete equations numerically. This method is a common mark of
Effective Field Theories. In the limit, when the small parameters are equal to 0, the post-Newtonian expansion reduces to Newton's law of gravity.