Concept record · Atlas v1.2.0
de Sitter conjecture
ConjectureWhat the term means here
The proposal that scalar potentials in any consistent quantum-gravity effective theory satisfy a gradient bound of the form |∇V| ≥ c·V, with c a positive number of order one in Planck units. Taken at face value it forbids stable de Sitter minima, where the gradient vanishes and V is positive.
Why it matters to this question
It converts a hard construction problem into a sharp, falsifiable-looking criterion, and it is the single statement around which the post-2018 debate organizes.
What this does not establish
The conjecture rests on asymptotic and thermodynamic arguments, not on a ten-dimensional proof. Critics argue that an order-one c is in tension with slow-roll inflation and with the observed value of Λ, and that the conjecture over-generalizes tree-level no-go theorems.
Claims bearing on this concept · 3
- ds-007
The de Sitter swampland conjecture proposes that scalar potentials in consistent quantum-gravity effective theories obey a gradient bound |∇V| ≥ c·V, with c of order one.
- ds-008
An order-one value of c has been argued to be in tension with slow-roll inflation and with the observed value of the cosmological constant.
- ds-009
The Trans-Planckian Censorship Conjecture proposes that sub-Planckian fluctuations never cross the Hubble horizon and freeze, which bounds the lifetime of a de Sitter phase.
Sources used for this record · 3
- The original de Sitter swampland conjecturearXiv:1806.08362
- The slow-roll bound supporting the conjecturearXiv:1807.05193
- Cosmological critique of the de Sitter conjecturearXiv:1808.09440