Pith. sign in

On de Sitter vacua in O(d,d) invariant cosmology

1 Pith paper cite this work. Polarity classification is still indexing.

1 Pith paper citing it
abstract

We perform a thorough analysis of de Sitter vacua in O(d,d) invariant cosmologies. Starting with a homogeneous and isotropic framework we examine conditions for the existence of such vacua, non-perturbative in \alpha' in both the string frame and the Einstein frame. We elucidate the nature of the instability in the string frame vacuum. For the Einstein frame, we demonstrate that the de Sitter vacuum cannot be eternal. We then extend our analysis to include Bianchi I universes where the O(d,d) symmetry includes scale factor exchange as well as scale factor duality. We show how the theory can be extended to the anisotropic case so that it admits de Sitter vacua, noting the crucial role played by the O(d,d) symmetry in satisfying any additional constraints.

citation-role summary

background 1

citation-polarity summary

fields

hep-th 1

years

2025 1

verdicts

CONDITIONAL 1

roles

background 1

polarities

unclear 1

representative citing papers

Higher co-dimension de Sitter branes

hep-th · 2025-06-24 · conditional · novelty 6.0

A no-go theorem shows that thin co-dimension-two branes cannot support de Sitter vacua in compactified supergravity, and higher co-dimensions need negative tension.

citing papers explorer

Showing 1 of 1 citing paper.

  • Higher co-dimension de Sitter branes hep-th · 2025-06-24 · conditional · none · ref 28 · internal anchor

    A no-go theorem shows that thin co-dimension-two branes cannot support de Sitter vacua in compactified supergravity, and higher co-dimensions need negative tension.