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Phys. Rev. D 16, 1601–1608 (1977)

Quantized gravitational wave perturbations in Robertson-Walker universes

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L. H. Ford and Leonard Parker
Department of Physics, University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201

Received 21 April 1977; published in the issue dated 15 September 1977

We consider the theory of quantized gravitational wave perturbations in the three types of Robertson-Walker universes. In a gauge analogous to the Coulomb gauge in electrodynamics it is possible to identify and quantize the independent degrees of freedom of the graviton field. The resulting theory is equivalent to that for a pair of massless, minimally coupled scalar fields in the same background space-time. As an application of the formalism, we calculate the spectrum of gravitons produced by a power-law expansion of the universe and show that it has no divergences.

© 1977 by The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.16.1601
DOI:
10.1103/PhysRevD.16.1601
PACS:

See Also

Comment: E. Gunzig and P. Nardone, Role of conformal (non) invariance in graviton production by cosmological background, Phys. Rev. D 19, 1275 (1979).