On the occurrence of finite-time singularities in swampland-related quintessence dark energy models

DOI10.1142/S0219887821502078arXiv2108.11324MaRDI QIDQ6118674

Unnamed Author, V. K. Oikonomou, Achilles Gitsis

Publication date: 21 March 2024

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2108.11324

zbMATH Keywords

cosmologyphase spacedynamical systems in cosmologyswampland criteria

Mathematics Subject Classification ID

Differential geometry (53-XX) Relativity and gravitational theory (83-XX)

Cites Work

• Swampland implications of GW170817-compatible Einstein-Gauss-Bonnet gravity
• Supersymmetric protection and the swampland
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• Do we live in the swampland?
• The multi-field, rapid-turn inflationary solution
• Quantum log-corrections to swampland conjectures
• Strengthening the De Sitter swampland conjecture in warm inflation
• Multi-field dark energy: cosmic acceleration on a steep potential
• AdS and the swampland
• Dark energy beyond quintessence: constraints from the swampland
• Hidden sectors in string theory: kinetic mixings, fifth forces and quintessence
• Rescaled Einstein–Hilbert gravity: Inflation and the Swampland criteria
• Hyperbolic field space and swampland conjecture for DBI scalar
• The string swampland constraints require multi-field inflation
• Runaway quintessence, out of the swampland
• Minimal gauge inflation and the refined Swampland conjecture
• The Landscape, the Swampland and the Era of Precision Cosmology
• Pixelated Dark Energy

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