1996
DOI: 10.1016/0370-2693(95)01519-1
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Maximally symmetric cosmological solutions of higher-curvature string effective theories with dilatons

Abstract: We study the effect of higher-curvature terms in the string low-energy effective actions on the cosmological solutions of the theory, up to corrections quartic in the curvatures, for the bosonic and heterotic strings as well as for the type II superstring. We find that cosmological solutions exist for all string types but they always disappear when the dilaton field is included, a conclusion that can be avoided if string-loop effects are taken into account.

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Cited by 113 publications
(96 citation statements)
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“…For two interesting examples we note a new non-singular cosmological attractor in String Gravity [25,26,27] and an ultimate bounce independent of initial conditions and a scalar field potential in Loop Quantum Cosmology [28] (for general descriptions of these theories, see, for example, [29,30,31,32]). …”
Section: A4 Anisotropic Universementioning
confidence: 99%
“…For two interesting examples we note a new non-singular cosmological attractor in String Gravity [25,26,27] and an ultimate bounce independent of initial conditions and a scalar field potential in Loop Quantum Cosmology [28] (for general descriptions of these theories, see, for example, [29,30,31,32]). …”
Section: A4 Anisotropic Universementioning
confidence: 99%
“…First, they can give useful insight as regards sensible implementations of string-motivated scenarios in the early-universe inflationary context [24,25]. Secondly, stable dS solutions may avoid the infall of the late universe in eventual finite-time singularities.…”
Section: Preliminary Remarks and Geometrical Inflationmentioning
confidence: 99%
“…Furthermore, at least up to order α ′3 , the structure of the higher order curvature terms does not allow, in the presence of the dilaton, for stable de Sitter type solutions [2]. However, there are some cases where a successful inflationary scenario can be developed as in the so-called dilaton-driven kinetic inflation or Pre-Big-Bang model [3] 1 or assuming that the dilaton has been stabilized and that the inflaton is a gauge singlet field other than the dilaton [7,8,9] .…”
mentioning
confidence: 99%