Quantum fine-tuning in stringy quintessence models

DOI10.1016/j.physletb.2019.134878zbMath1427.83104arXiv1812.03184OpenAlexW2904586784MaRDI QIDQ2281123

Mark Trodden, Mark P. Hertzberg, McCullen Sandora

Publication date: 19 December 2019

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1812.03184

Mathematics Subject Classification ID

String and superstring theories in gravitational theory (83E30)

Related Items

Multi-field inflation in high-slope potentials ⋮ Non-canonical kinetic structures in the swampland ⋮ The Swampland: Introduction and Review ⋮ Pixelated Dark Energy ⋮ Reconstruction of quintessence field for the THDE with swampland correspondence in f(R,T) gravity ⋮ Multi-field dark energy: cosmic acceleration on a steep potential ⋮ The \(F\)-term problem and other challenges of stringy quintessence ⋮ Hyperbolic field space and swampland conjecture for DBI scalar ⋮ Conditions for (no) eternal inflation

Cites Work

• Inflationary constraints on type IIA string theory
• On the geometry of the string landscape and the swampland
• SUPERGRAVITY DESCRIPTION OF FIELD THEORIES ON CURVED MANIFOLDS AND A NO GO THEOREM
• Mirror dark matter: Cosmology, galaxy structure and direct detection
• Fixing moduli in exact Type IIA flux vacua