Two‐Field Axion Inflation and the Swampland Constraint in the Flux‐Scaling Scenario

DOI10.1002/prop.201800072arXiv1808.03397OpenAlexW2949638815WikidataQ128855346 ScholiaQ128855346MaRDI QIDQ6063923

Cesar Damian, Oscar Loaiza-Brito

Publication date: 8 November 2023

Published in: Fortschritte der Physik (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1808.03397

zbMATH Keywords

swamplandmultifield inflationflux scaling scenario

Mathematics Subject Classification ID

Quantum theory (81-XX)

Related Items (9)

Constraints on dark energy models from the Horndeski theory ⋮ Multi-field inflation in high-slope potentials ⋮ On the weak gravity conjecture in string theory with broken supersymmetry ⋮ 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 ⋮ Dark energy and the refined De Sitter conjecture ⋮ Leaving the Swampland: non-geometric fluxes and the distance conjecture ⋮ Hyperbolic field space and swampland conjecture for DBI scalar

Cites Work

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• Type IIB flux vacua from G-theory. II
• Supersymmetric moduli stabilization and high-scale inflation
• Universal ds vacua in STU-models
• The Flux-Scaling scenario: De sitter uplift and axion inflation
• Double field theory: a pedagogical review
• Inflation, Cosmic Perturbations and Non-Gaussianities
• Inflationary universe: A possible solution to the horizon and flatness problems
• Lectures on nongeometric flux compactifications
• On Inflation and de Sitter in Non‐Geometric String Backgrounds

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