Non-canonical kinetic structures in the swampland

DOI10.1088/1475-7516/2020/09/049zbMath1493.83033arXiv2004.09526OpenAlexW3017546239MaRDI QIDQ5070957

Adam R. Solomon, Mark Trodden

Publication date: 14 April 2022

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

Full work available at URL: https://arxiv.org/abs/2004.09526

zbMATH Keywords

inflationcosmology of theories beyond the SMparticle physics-cosmology connectionstring theory and cosmology

Mathematics Subject Classification ID

Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) Spectrum, resolvent (47A10) Quantum field theory on curved space or space-time backgrounds (81T20) Geometrodynamics and the holographic principle (83E05) Constrained dynamics, Dirac's theory of constraints (70H45) Effective quantum field theories (81T12)

Related Items (3)

Positivity vs. Lorentz-violation: an explicit example ⋮ Multi-field dark energy: cosmic acceleration on a steep potential ⋮ Partial UV completion of P(X) from a curved field space

Cites Work

• Quantum corrections and the de Sitter swampland conjecture
• On the geometry of the string landscape and the swampland
• Degenerate higher order scalar-tensor theories beyond Horndeski up to cubic order
• The effective field theory of cosmological large scale structures
• Quantum fine-tuning in stringy quintessence models
• Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
• Higher-derivative operators and effective field theory for general scalar-tensor theories
• Recovering P(X) from a canonical complex field
• Consistency of tachyacoustic cosmology with de Sitter swampland conjectures
• Keeping an eye on DBI: power-counting for small-c_s cosmology
• Hyperbolic field space and swampland conjecture for DBI scalar
• The string swampland constraints require multi-field inflation
• \(k\)-inflation
• The Landscape, the Swampland and the Era of Precision Cosmology

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