On the superstrings-induced four-dimensional gravity, and its applications to cosmology
arXiv:0707.3359 · doi:10.1155/2008/521389
Abstract
We review the status of the fourth-order (quartic in the spacetime curvature) terms induced by superstrings/M-theory (compactified on a warped torus) in the leading order with respect to the Regge slope parameter, and study their (non-perturbative) impact on the evolution of the Hubble scale in the context of the four-dimensional FRW cosmology. After taking into account the quantum ambiguities in the definition of the off-shell superstring effective action, we propose the generalized Friedmann equations, find the existence of their (de Sitter) exact inflationary solutions without a spacetime singularity, and constrain the ambiguities by demanding stability and the scale factor duality invariance of our solutions. The most naive (Bel-Robinson tensor squared) quartic terms are ruled out, thus giving the evidence for the necessity of extra quartic (Ricci tensor-dependent) terms in the off-shell gravitational effective action for superstrings. Our methods are generalizable to the higher orders in the spacetime curvature.
33 pages, LaTeX, no figures; extensive revision, Sec.6 and references added, stability analysis included
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Cited by in corpus (10)
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- Fourth-order gravity as the inflationary model revisited
- On the superstring-inspired quantum correction to the Starobinsky model of inflation
- Slow-roll inflation in (R+R*4) gravity
- F(R) supergravity
- Scalar potential in F(R) supergravity
- Stability investigations of isotropic and anisotropic exponential inflation in the Starobinsky-Bel-Robinson gravity
- Starobinsky inflation beyond the leading order
- Einstein-Grisaru-Zanon gravity
- Starobinsky-Bel-Robinson gravity