Primordial Spectral Indices from Generalized Einstein Theories
arXiv:astro-ph/9408044 · doi:10.1103/PhysRevD.52.4295
Abstract
Primordial spectral indices are calculated to second order in slow-roll parameters for three closely-related models of inflation, all of which contain a scalar field non-minimally coupled to the Ricci curvature scalar. In most cases, may be written as a function of the non-minimal curvature coupling strength alone, with , although the constraints on differ greatly between \lq new inflation' and \lq chaotic inflation' initial conditions. Under \lq new inflation' initial conditions, there are discrepancies between the values of as calculated in the Einstein frame and the Jordan frame. The sources for these discrepancies are addressed, and shown to have negligible effects on the numerical predictions for . No such discrepancies affect the calculations under \lq chaotic inflation' initial conditions.
31 pp. Forthcoming in Physical Review D. Section 3 significantly revised. Four figures not included; hard copies available from author
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