A navigable, source-first guide to the de Sitter problem in string theory. It maps how the concepts connect, labels how well each claim is supported, and sends you to the primary literature rather than standing in for it.
Educational research map · non-peer-reviewed orientation tool
Built from The de Sitter Problem in the String Swampland: A Verified Literature Map (v2.0, 2026-07-26), archived at DOI 10.5281/zenodo.21603961 (concept DOI 10.5281/zenodo.21603960). Every source below is drawn from that paper’s verified citation set. String theory and M-theory are research frameworks; neither is an experimentally confirmed description of nature, and nothing here should be read as claiming otherwise.
A label describes the standing of a claim, not its importance. Nothing on this page is labelled “established” unless the source material supports that distinction — which here means a defined mathematical construction or a published laboratory measurement, never the question of whether de Sitter vacua exist in string theory.
Select a concept to open its definition, epistemic status, and sources. Arrows show the direction of dependence or derivation, not agreement — several of them mark exactly where the field disagrees. Press Esc to close the panel.
No concept selected. Choose one from the map above to see its definition, why it matters, its epistemic status, and its sources.
Each claim is stated in careful language, labelled, explained, sourced to the working paper’s verified citation set, and paired with the limitation that keeps it honest. Read the caution before quoting the claim.
The observed late-time acceleration of the universe is standardly modeled with a small positive cosmological constant, and current data place the dark-energy equation of state near w = −1.
Whether string/M-theory admits stable or metastable de Sitter vacua remains an open question, and there is no community consensus.
KKLT is a specific, well-defined proposal for obtaining a de Sitter vacuum: flux and non-perturbative stabilization into a supersymmetric anti-de Sitter minimum, followed by an anti-D3-brane uplift.
Whether the KKLT anti-brane uplift is under parametric ten-dimensional supergravity control is actively debated.
The Large Volume Scenario stabilizes Kähler moduli at exponentially large volume, which nominally suppresses α′ and loop corrections.
It has been argued that keeping LVS de Sitter constructions under control requires a negative D3-tadpole exceeding known Calabi-Yau bounds.
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.
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.
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.
If metastable de Sitter vacua are excluded, dark energy would have to be dynamical — a rolling scalar field rather than a constant.
The Dark Dimension scenario ties the dark-energy scale to a Kaluza-Klein scale via the AdS distance conjecture, predicting a single extra dimension of roughly micron size.
Torsion-balance experiments report no deviation from the gravitational inverse-square law down to separations of about 52 micrometres.
This is a curated orientation layer. It exists to get you to the point where you can read the primary literature yourself, and then to get out of the way. It is not a substitute for those papers, not expert advice, and not a statement of scientific consensus — on the central question it maps, there is no consensus to state.
Two nodes, Holography and Observational cosmology, are included for orientation but are not cited directly in the source map. They are marked as such, and no citation has been attached to them that the source does not support.
There is no chat interface here by design. A retrieval layer that paraphrases contested physics is precisely the tool most likely to flatten a live disagreement into a confident answer.
Every work cited on this page, drawn without exception from the working paper. Entries marked foundational are cited there by journal reference or identifier only; where the paper records no title, none is supplied here.