The Einstein-Hilbert action is given by,
I=116πG∫Mddx√−gR+18πG∫∂Mdd−1x√−hK
including the Gibbons-Hawking-York boundary term. A well-known derivation of the entropy of the Schwarzschild metric requires the evaluation of the boundary term. However, one must introduce a radial regulator R, and subtract off a counter-term which is the Gibbons-Hawking action of emtpy space with the same boundary. The final result is finite as R→∞.
I am attempting to calculate the full action for a solution for which R≠0, hence I need to also compute the pure Einstein-Hilbert piece. However, I must introduce a regulator, and the final action is not finite as I take it to infinity. My question: is there an analogous procedure to "tame" the infinity of the pure Einstein-Hilbert piece, perhaps similar to the treatment of the Gibbons-Hawking term?
I actually have to introduce two regulators. For my solution, the Ricci scalar is independent of a particular coordinate, x1, so I get a factor of x1 after integration evaluated at ±∞, so I introduced regulators, such that L−<x1<L+. As I take L±→±∞, of course it is divergent.
This post imported from StackExchange Physics at 2014-05-04 11:36 (UCT), posted by SE-user user2062542