A new light on the darkest corner of the landscape
arXiv:1810.11365
Abstract
Motivated by the recently proposed bounds on the slow-roll parameters for scalar potentials arising from string/M-theory compactifications, a.k.a. the Refined de Sitter Swampland conjecture, we explore the sharpness of such constraints within 4D supergravities coming from compactifications of massive type IIA string theory on . With the aid of a numerical technique, known as differential evolution, we are able to find a de Sitter extremum which is fully metastable up to one single flat direction. This solution is supported by spacetime filling sources such as O6 planes and KK monopoles. Our example violates the bound imposed by this conjecture.
13 pages, 2 figures, 6 tables
References in corpus (7)
- Distance and de Sitter Conjectures on the Swampland
- Simple de Sitter Solutions
- Bounds on Slow Roll at the Boundary of the Landscape
- A second look at N=1 supersymmetric AdS_4 vacua of type IIA supergravity
- Algebras and non-geometric flux vacua
- Beyond Twisted Tori
- A second look at gauged supergravities from fluxes in M-theory
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