Casimir-stabilized AdS vacua with parametric scale separation in supergravity exhibit perturbative and non-perturbative instabilities under deformations.
Bubble needs strings
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
fields
hep-th 3verdicts
UNVERDICTED 3roles
background 1polarities
background 1representative citing papers
The dark bubble model realizes the dark dimension and fat graviton proposals by predicting a micron-sized extra dimension, gravity weakening at that scale, a tens-of-TeV string scale, and measurable positive spatial curvature.
String theory imposes constraints on dark energy but permits various construction attempts for de Sitter vacua and single-field exponential quintessence models despite obstructions.
citing papers explorer
-
Instabilities in scale-separated Casimir vacua
Casimir-stabilized AdS vacua with parametric scale separation in supergravity exhibit perturbative and non-perturbative instabilities under deformations.