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- W2953641188 endingPage "040" @default.
- W2953641188 startingPage "040" @default.
- W2953641188 abstract "We have presented previously a general treatment of Starobinsky-like inflation in no-scale supergravity where the tensor-to-scalar ratio r = 3(1 − ns)2, and ns is the tilt of the scalar perturbations. In particular, we have shown how this scenario can be unified with modulus fixing, supersymmetry breaking and a small cosmological constant. In this paper we extend these constructions to inflationary models based on generalized no-scale structures. In particular, we consider alternative values of the curvature parameter, α < 1, as may occur if not all the complex Kähler moduli contribute to driving inflation, as well as α > 1, as may occur if complex structure moduli also contribute to driving inflation. In all cases, we combine these α-Starobinsky inflation models with supersymmetry breaking and a present-day cosmological constant, allowing for additional contributions to the vacuum energy from stages of gauge symmetry breaking." @default.
- W2953641188 created "2019-07-12" @default.
- W2953641188 creator A5020965685 @default.
- W2953641188 creator A5052011846 @default.
- W2953641188 creator A5075475814 @default.
- W2953641188 creator A5081403178 @default.
- W2953641188 date "2019-09-20" @default.
- W2953641188 modified "2023-09-23" @default.
- W2953641188 title "Unified no-scale attractors" @default.
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