Renormalization of higher-derivative quantum gravity
Gravitational actions which include terms quadratic in the curvature tensor are renormalizable. The necessary Slavnov identities are derived from Becchi-Rouet-Stora (BRS) transformations of the gravitational and Faddeev-Popov ghost fields. In general, non-gauge-invariant divergences do arise, but they may be absorbed by nonlinear renormalizations of the gravitational and ghost fields (and of the BRS transformations). Fortunately, these artifactual divergences may be eliminated by letting the coefficients of the harmonic-gauge-fixing term tend to infinity, thus considerably simplifying the renormalization procedure. Coupling to other renormalizable fields may then be handled in a straightforward manner.
- Research Organization:
- Department of Physics, Brandeis University, Waltham, Massachusetts 02154
- OSTI ID:
- 7209746
- Journal Information:
- Phys. Rev., D; (United States), Journal Name: Phys. Rev., D; (United States) Vol. 16:4; ISSN PRVDA
- Country of Publication:
- United States
- Language:
- English
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657003 -- Theoretical & Mathematical Physics-- Relativity & Gravitation
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
DIAGRAMS
EQUATIONS
FADDEEV EQUATIONS
FEYNMAN DIAGRAM
FIELD THEORIES
GAUGE INVARIANCE
GRAVITATIONAL FIELDS
INVARIANCE PRINCIPLES
METRICS
PROPAGATOR
QUANTUM FIELD THEORY
RENORMALIZATION
RICCI TENSOR
SCALAR FIELDS
TENSORS