Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
2010-05-25
Phys.Rev.D82:043501,2010
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
31 pages, 1 figure, uses LaTeX2epsilon
Scientific paper
10.1103/PhysRevD.82.043501
We discuss the additional perturbation introduced during inflation by quantum stress tensor fluctuations of a conformally invariant field such as the photon. We consider both a kinematical model, which deals only with the expansion fluctuations of geodesics, and a dynamical model which treats the coupling of the stress tensor fluctuations to a scalar inflaton. In neither model do we find any growth at late times, in accordance with a theorem due to Weinberg. What we find instead is a correction which becomes larger the earlier one starts inflation. This correction is non-Gaussian and highly scale dependent, so the absence of such effects from the observed power spectra may imply a constraint on the total duration of inflation. We discuss different views about the validity of perturbation theory at very early times during which currently observable modes are transplanckian.
Ford L. H.
Miao Shun-Pei
Ng Kin-Wang
Woodard Richard P.
Wu Chun-Hsien
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