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New non-perturbative de Sitter vacua in α′-complete cosmology

Carmen A. Núñez, Facundo Emanuel Rost

2021Journal of High Energy Physics30 citationsDOIOpen Access PDF

Abstract

A bstract The α′ -complete cosmology developed by Hohm and Zwiebach classifies the O( d, d ; ℝ) invariant theories involving metric, b -field and dilaton that only depend on time, to all orders in α′ . Some of these theories feature non-perturbative isotropic de Sitter vacua in the string frame, generated by the infinite number of higher-derivatives of O( d, d ; ℝ) multiplets. Extending the isotropic ansatz, we construct stable and unstable non-perturbative de Sitter solutions in the string and Einstein frames. The generalized equations of motion admit new solutions, including anisotropic d + 1-dimensional metrics and non-vanishing b -field. In particular, we find dS n +1 × T d−n geometries with constant dilaton, and also metrics with bounded scale factors in the spatial dimensions with non-trivial b -field. We discuss the stability and non-perturbative character of the solutions, as well as possible applications.

Topics & Concepts

PhysicsDe Sitter universeDilatonIsotropyTheoretical physicsExtra dimensionsMathematical physicsBounded functionString theoryAnti-de Sitter spaceInvariant (physics)Cosmological constantString cosmologyCosmologyEquations of motionEinsteinScale invarianceClassical mechanicsKaluza–Klein theoryString (physics)De Sitter spaceCompactification (mathematics)AnisotropyGravitonde Sitter invariant special relativityBrane cosmologyStability (learning theory)Motion (physics)Cosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsNoncommutative and Quantum Gravity Theories
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