A Note on Inflation and the Swampland

DOI10.1002/prop.201800052arXiv1807.05445OpenAlexW2884327748WikidataQ129388393 ScholiaQ129388393MaRDI QIDQ6084548

Alex Kehagias, Antonio Riotto

Publication date: 6 November 2023

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

Full work available at URL: https://arxiv.org/abs/1807.05445

zbMATH Keywords

inflationswampland

Mathematics Subject Classification ID

Quantum theory (81-XX)

Related Items (15)

Constraints on dark energy models from the Horndeski theory ⋮ Consistency of tachyacoustic cosmology with de Sitter swampland conjectures ⋮ Multi-field inflation in high-slope potentials ⋮ Eternal inflation in swampy landscapes ⋮ Topological eternal hilltop inflation and the swampland criteria ⋮ Multi-field cold and warm inflation and the de Sitter swampland conjectures ⋮ Hidden sectors in string theory: kinetic mixings, fifth forces and quintessence ⋮ Scaling limits of ds vacua and the swampland ⋮ (Super)universal attractors and the de Sitter vacua in string landscape ⋮ Compact objects and the swampland ⋮ Inflationary Cosmology with Quantum Gravitational Effects and Swampland Conjectures* ⋮ Dark energy beyond quintessence: constraints from the swampland ⋮ Dark energy and the refined De Sitter conjecture ⋮ Hyperbolic field space and swampland conjecture for DBI scalar ⋮ f(R) and Brans-Dicke theories and the Swampland

Cites Work

• On the geometry of the string landscape and the swampland
• Infinite distances in field space and massless towers of states
• On the de Sitter swampland criterion
• What if string theory has no de Sitter vacua?
• Inflationary universe: A possible solution to the horizon and flatness problems
• The string swampland constraints require multi-field inflation

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