skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Quantum stress tensor fluctuations of a conformal field and inflationary cosmology

Journal Article · · Physical Review. D, Particles Fields
 [1];  [2];  [3];  [4];  [3]
  1. Institute of Cosmology, Department of Physics and Astronomy, Tufts University, Medford, Massachusetts 02155 (United States)
  2. Centro de Estudios Cientificos (CECS), Casilla 1469, Valdivia (Chile)
  3. Institute of Physics, Academia Sinica, Nankang, Taipei 11529, Taiwan (China)
  4. Department of Physics, University of Florida, Gainesville, Florida 32611 (United States)

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 trans-Planckian.

OSTI ID:
21420908
Journal Information:
Physical Review. D, Particles Fields, Vol. 82, Issue 4; Other Information: DOI: 10.1103/PhysRevD.82.043501; (c) 2010 The American Physical Society; ISSN 0556-2821
Country of Publication:
United States
Language:
English