arXiv:gr-qc/0411003·v2·General Relativity and Quantum Cosmology
Stress Tensor Correlators in the Schwinger-Keldysh Formalism
L. H. Ford (Tufts University)🇺🇸 · R. P. Woodard (University of Florida)🇺🇸
Abstract
We express stress tensor correlators using the Schwinger-Keldysh formalism. The absence of off-diagonal counterterms in this formalism ensures that the +- and -+ correlators are free of primitive divergences. We use dimensional regularization in position space to explicitly check this at one loop order for a massless scalar on a flat space background. We use the same procedure to show that the ++ correlator contains the divergences first computed by `t Hooft and Veltman for the scalar contribution to the graviton self-energy.
Comments: 14 pages, LaTeX 2epsilon, no figures, revised for publication