Semiclassical gravity in the far field limit of stars, black holes, and wormholes

P. R. A. would like to thank R. Wald and L. Ford for helpful comments. P. R. A., A. F., and S. F. would like to thank R. Balbinot for helpful discussions. The work of P. R. A. was supported in part by the National Science Foundation under Grant Nos. PHY-0556292 and PHY-0856050. A. F. acknowledges financial support by Generalitat Valenciana and MICINN Grant No. FIS2008-06078-C03-02. Numerical computations were performed on the Wake Forest University DEAC Cluster with support from an IBM SUR grant and the Wake Forest University IS Department. Computational results were supported by storage hardware supplied to Wake Forest University through an IBM SUR grant.