Renormalized graviton stress-energy tensor in curved vacuum space-times

B. Allen, A. Folacci, and A. C. Ottewill
Phys. Rev. D 38, 1069 – Published 15 August 1988
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Abstract

The graviton contribution to the renormalized one-loop effective stress-energy tensor is calculated in an arbitrary vacuum space-time with a cosmological constant. This is done for (1) the standard definition of the effective action and (2) the reparametrization-invariant effective action of Vilkovisky and DeWitt. The renormalized one-loop effective stress-energy tensor is given in terms of the graviton two-point function, by making use of its symmetric Hadamard representation.

  • Received 3 December 1987

DOI:https://doi.org/10.1103/PhysRevD.38.1069

©1988 American Physical Society

Authors & Affiliations

B. Allen, A. Folacci, and A. C. Ottewill

  • Groupe d’Astrophysique Relativiste, Centre National de la Recherche Scientifique, Observatoire de Paris(enMeudon, 92195 Meudon, France

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Vol. 38, Iss. 4 — 15 August 1988

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