Higher order terms in the inflaton potential and the lower bound on the tensor to scalar ratio \(r\)

DOI10.1016/J.AOP.2010.11.019zbMath1213.83143arXiv0906.4102OpenAlexW2095821488MaRDI QIDQ2431314

H. J. De Vega, N. G. Sánchez, Claudio Destri

Publication date: 13 April 2011

Published in: Annals of Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0906.4102

zbMATH Keywords

inflationCMB anisotropieseffective field theory à la Ginsburg-Landauprimordial gravitons

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Radiative transfer in astronomy and astrophysics (85A25) Astrophysical cosmology (85A40)

Related Items (1)

Inflationary predictions of double-well, Coleman-Weinberg, and hilltop potentials with non-minimal coupling

Cites Work

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• THE EFFECTIVE THEORY OF INFLATION IN THE STANDARD MODEL OF THE UNIVERSE AND THE CMB+LSS DATA ANALYSIS
• The Primordial Density Perturbation

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