English

New non-perturbative de Sitter vacua in $\alpha'$-complete cosmology

High Energy Physics - Theory 2021-03-17 v2

Abstract

The α\alpha'-complete cosmology developed by Hohm and Zwiebach classifies the O(d,d;R){\rm O}(d,d;{\mathbb R}) invariant theories involving metric, bb-field and dilaton that only depend on time, to all orders in α\alpha'. 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){\rm O}(d,d;{\mathbb 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+1d+1-dimensional metrics and non-vanishing bb-field. In particular, we find dSn+1×Tdn_{n+1}\times T^{d-n} geometries with constant dilaton, and also metrics with bounded scale factors in the spatial dimensions with non-trivial bb-field. We discuss the stability and non-perturbative character of the solutions, as well as possible applications.

Keywords

Cite

@article{arxiv.2011.10091,
  title  = {New non-perturbative de Sitter vacua in $\alpha'$-complete cosmology},
  author = {Carmen A. Núñez and Facundo Emanuel Rost},
  journal= {arXiv preprint arXiv:2011.10091},
  year   = {2021}
}

Comments

52 pages, 2 figures; v2: 53 pages, 2 figures, discussions, references and acknowledgements added

R2 v1 2026-06-23T20:22:56.665Z