On the de Sitter swampland criterion

From MaRDI portal
Publication:1989776

DOI10.1016/j.physletb.2018.09.022zbMath1398.83116arXiv1806.10999OpenAlexW2810691270MaRDI QIDQ1989776

David Andriot

Publication date: 29 October 2018

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1806.10999




Related Items (70)

The entropic quasi-de Sitter instability time from the distance conjectureThe unbearable lightness of charged gravitiniDe Sitter quantum breaking, swampland conjectures and thermal stringsDe Sitter and anti-de Sitter branes in self-tuning modelsNatural chain inflationInstability of de Sitter space under thermal radiation in different vacuaTrans-Planckian Censorship and single-field inflaton potentialA tip for landscape riders: multi-field inflation can fulfill the swampland distance conjectureMulti-field inflation in high-slope potentialsEternal inflation in swampy landscapesTopological eternal hilltop inflation and the swampland criteriaWarm dark energyOut of the swampland with multifield quintessence?De Sitter in non-supersymmetric string theories: no-go theorems and brane-worldsConifold dynamics and axion monodromiesSwampland constraints on no-boundary quantum cosmologySystematics of type IIA moduli stabilisationOn the weak gravity conjecture in string theory with broken supersymmetryQuantum log-corrections to swampland conjecturesOn/off scale separationAnti-brane uplift instability from goldstino condensationExploring the landscape of (anti-) de Sitter and Minkowski solutions: group manifolds, stability and scale separationDe Sitter vs Quintessence in String Theoryde Sitter Extrema and the SwamplandQuantum Breaking Bound on de Sitter and SwamplandNew Constraints on Classical de Sitter: Flirting with the SwamplandHidden sectors in string theory: kinetic mixings, fifth forces and quintessenceScaling limits of ds vacua and the swamplandWeakly coupled de Sitter vacua with fluxes and the swamplandA holographic derivation of the weak gravity conjecture(In)stability of de Sitter vacuum in light of distance conjecture and emergence proposalThe quantum swamplandA Note on Inflation and the SwamplandReference Level of the Vacuum Energy Density of the Universe and Astrophysical DataHiggs in nilpotent supergravity: vacuum energy and Festina LenteQuantum gravity constraints on scale separation and de Sitter in five dimensionsNegative scalar potentials and the swampland: an anti-trans-Planckian censorship conjectureBeginners lectures on flux compactifications and related swampland topicsBounds on tower mass scales in the presence of throats of different warpingComments on the transplanckian censorship conjectureAutomated consistent truncations and stability of flux compactifications(Quasi-) de Sitter solutions across dimensions and the TCC boundDo we live in the swampland?The web of swampland conjectures and the TCC boundNew de Sitter solutions of 10d type IIB supergravityNew de Sitter solutions in ten dimensions and orientifold singularitiesQuantum corrections and the de Sitter swampland conjectureRacetrack potentials and the de Sitter swampland conjecturesTrans-Planckian censorship and the swamplandA strong scalar weak gravity conjecture and some implicationsOh, wait, O8 de Sitter may be unstable!Weak gravity versus de SitterThe gravitino and the swamplandOn stringy De Sitter spacetimesDark energy beyond quintessence: constraints from the swamplandDark energy and the refined De Sitter conjectureModular symmetries and the swampland conjecturesSwampland variations on a theme by KKLTA ds obstruction and its phenomenological consequencesdS spaces and brane worlds in exotic string theoriesSharpening the boundaries between flux landscape and swampland by tadpole chargeConstructing stable De Sitter in M-theory from higher curvature correctionsCharting the landscape of (anti-) de Sitter and Minkowski solutions of 10d supergravitiesType IIB flux compactifications with \(h^{1, 1} = 0\)Hyperbolic field space and swampland conjecture for DBI scalarThe string swampland constraints require multi-field inflationf(R) and Brans-Dicke theories and the SwamplandO6-plane backreaction on scale-separated type IIA \(\mathrm{AdS}_3\) vacuaSmall-field and scale-free: inflation and ekpyrosis at their extremesConditions for (no) eternal inflation



Cites Work


This page was built for publication: On the de Sitter swampland criterion