Feynman propagator in curved spacetime: A momentum-space representation
We obtain a momentum-space representation of the Feynman propagator G (x,x') for scalar and spin-1/2 fields propagating in arbitrary curved spacetimes. The construction uses Riemann normal coordinates with origin at the point x' and is therefore only valid for points x lying in a normal neighborhood of x'. We show that the resulting momentum-space representation is equivalent to the DeWitt-Schwinger proper-time representation. Our momentum-space representation permits one to apply momentum-space techniques used in Minkowski space to arbitrary curved spacetimes. The usefulness of this representation in discussing the renormalizability of interacting field theories in curved spacetime is illustrated by an explicit renormalization, to second order in the coupling constant, of a quartically self-interacting scalar field theory in an arbitrary spacetime.
- Research Organization:
- Department of Physics, University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201
- OSTI ID:
- 5727546
- Journal Information:
- Phys. Rev., D; (United States), Vol. 20:10
- Country of Publication:
- United States
- Language:
- English
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71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
FEYNMAN PATH INTEGRAL
PROPAGATOR
FIELD THEORIES
RENORMALIZATION
SCALAR FIELDS
SPACE-TIME
COUPLING CONSTANTS
FIELD EQUATIONS
GREEN FUNCTION
METRICS
MINKOWSKI SPACE
SPIN
ULTRAVIOLET DIVERGENCES
ANGULAR MOMENTUM
EQUATIONS
FUNCTIONS
INTEGRALS
MATHEMATICAL SPACE
PARTICLE PROPERTIES
SPACE
645400* - High Energy Physics- Field Theory
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