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Cosmological attractors from<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>α</mml:mi></mml:math>-scale supergravity

Diederik RoestTheoretical High Energy PhysicsMarco ScalisiVan Swinderen Institute for Particle Physics and Gravity, University of Groningen, Nijenborgh 4, 9747 AG Groningen, Netherlands
2015lv
ABI

Аннотация

The Planck value of the spectral index can be interpreted as ${n}_{s}=1\ensuremath{-}2/N$ in terms of the number of $e$-foldings $N$. An appealing explanation for this phenomenological observation is provided by $\ensuremath{\alpha}$-attractors: the inflationary predictions of these supergravity models are fully determined by the curvature of the K\"ahler manifold. We provide a novel formulation of $\ensuremath{\alpha}$-attractors which only involves a single chiral superfield. Our construction involves a natural deformation of no-scale models and employs these to construct a de Sitter plateau with an exponential falloff. Finally, we show how analogous structures with a flat K\"ahler geometry arise as a singular limit of such $\ensuremath{\alpha}$-scale models.

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Цитирований: 3Использованных источников: 0