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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3091

Title: On the quasi-de sitter cosmological model of Starobinsky
Authors: Pollock, M.D.
Issue Date: Jun-1987
Publisher: Elsevier B.V.
Citation: Physics Letters B, 1987, Vol.192, p59-64
Abstract: A non-singular cosmological model that permits inflation has been constructed by Starobinsky, starting from the theory with lagrangian density Image. The spectrum of density perturbations is approximately adiabatic, with amplitude δρ/ρ≈|0−4 on the scale of a galaxy, provide that mless-than-or-equals, slant5×10−6mP. We rederive this constraint via the result of Whitt, who found by conformally transforming the metric that Image can be written in the form of gravity interacting with a minimally coupled scalar field. The implications of this result for the problem of initial conditions in the universe are also discussed.
Description: Restricted Access.
URI: http://hdl.handle.net/2289/3091
ISSN: 0370-2693
Alternative Location: http://dx.doi.org/10.1016/0370-2693(87)91142-7
Copyright: 1987 Elsevier B.V.
Appears in Collections:Research Papers (TP)

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