New Constraints on Classical de Sitter: Flirting with the Swampland
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Publication:6063935
DOI10.1002/prop.201800103arXiv1807.09698OpenAlexW2884904542MaRDI QIDQ6063935
Publication date: 8 November 2023
Published in: Fortschritte der Physik (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1807.09698
Related Items (22)
Multi-field inflation in high-slope potentials ⋮ Topological eternal hilltop inflation and the swampland criteria ⋮ De Sitter in non-supersymmetric string theories: no-go theorems and brane-worlds ⋮ Systematics of type IIA moduli stabilisation ⋮ On the weak gravity conjecture in string theory with broken supersymmetry ⋮ On asymptotic dark energy in string theory ⋮ Exploring the landscape of (anti-) de Sitter and Minkowski solutions: group manifolds, stability and scale separation ⋮ Hidden sectors in string theory: kinetic mixings, fifth forces and quintessence ⋮ Scaling limits of ds vacua and the swampland ⋮ Weakly coupled de Sitter vacua with fluxes and the swampland ⋮ A holographic derivation of the weak gravity conjecture ⋮ The quantum swampland ⋮ (Quasi-) de Sitter solutions across dimensions and the TCC bound ⋮ Universal accelerating cosmologies from 10d supergravity ⋮ The web of swampland conjectures and the TCC bound ⋮ New de Sitter solutions of 10d type IIB supergravity ⋮ On the de Sitter swampland criterion ⋮ Trans-Planckian censorship and the swampland ⋮ Obstacles to constructing de Sitter space in string theory ⋮ Spinors in supersymmetric dS/CFT ⋮ Consistent truncation and De Sitter space from gravitational instantons ⋮ Charting the landscape of (anti-) de Sitter and Minkowski solutions of 10d supergravities
Cites Work
- The four-point correlator in multifield inflation, the operator product expansion and the symmetries of de Sitter
- On the de Sitter swampland criterion
- SUPERGRAVITY DESCRIPTION OF FIELD THEORIES ON CURVED MANIFOLDS AND A NO GO THEOREM
- De Sitter hunting in a classical landscape
- What if string theory has no de Sitter vacua?
- Small-field and scale-free: inflation and ekpyrosis at their extremes
- The string swampland constraints require multi-field inflation
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