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Phys. Rev. D 48, 3677–3694 (1993)

Renormalization group for nonrenormalizable theories: Einstein gravity with a scalar field

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A. O. Barvinsky
Theoretical Physics Institute, Department of Physics, University of Alberta, Edmonton, Canada T6G 2J1
Nuclear Safety Institute, Russian Academy of Sciences, Bolshaya Tulskaya 52, Moscow 113191, Russia

A. Yu. Kamenshchik and I. P. Karmazin
Nuclear Safety Institute, Russian Academy of Sciences, Bolshaya Tulskaya 52, Moscow 113191, Russia

Received 30 June 1993; published in the issue dated 15 October 1993

We develop a renormalization-group formalism for nonrenormalizable theories and apply it to Einstein gravity theory coupled to a scalar field with the Lagrangian L= √g [RU(φ)-1/2G(φ)gμνμφνφ -V(φ)], where U(φ), G(φ), and V(φ) are arbitrary functions of the scalar field. We calculate the one-loop counterterms of this theory and obtain a system of renormalization-group equations in partial derivatives for the functions U, G, and V playing the role of generalized charges which substitute for the usual charges in multicharge theories. In the limit of a large but slowly varying scalar field and small spacetime curvature this system gives the asymptotic behavior of the generalized charges compatible with the conventional choice of these functions in quantum cosmological applications. It also demonstrates in the over-Planckian domain the existence of the Weyl-invariant phase of gravity theory asymptotically free in gravitational and cosmological constants.

© 1993 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.48.3677
DOI:
10.1103/PhysRevD.48.3677
PACS:
04.60.+n, 98.80.Hw