Multi-field cold and warm inflation and the de Sitter swampland conjectures

DOI10.1088/1475-7516/2022/09/001OpenAlexW4294192800WikidataQ122908689 ScholiaQ122908689MaRDI QIDQ5104206

Paulo M. Sá, Orfeu Bertolami

Publication date: 9 September 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2204.13794

zbMATH Keywords

inflationstring theory and cosmology

Mathematics Subject Classification ID

Geometrodynamics and the holographic principle (83E05) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30) Cut-elimination and normal-form theorems (03F05)

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Cites Work

• On the geometry of the string landscape and the swampland
• Inflation, phase transitions and the cosmological constant
• Strengthening the De Sitter swampland conjecture in warm inflation
• de Sitter vacua in string theory
• Was Einstein right?
• The Primordial Density Perturbation
• The string swampland constraints require multi-field inflation
• The Landscape, the Swampland and the Era of Precision Cosmology
• Further Refining the de Sitter Swampland Conjecture
• The Swampland: Introduction and Review
• A Note on Inflation and the Swampland