POST-INFLATION INCREASE OF THE COSMOLOGICAL TENSOR-TO-SCALAR PERTURBATION RATIO

DOI10.1142/S0217732305019122zbMath1082.83510arXivastro-ph/0507573MaRDI QIDQ5715653

Nicola Bartolo, Edward W. Kolb, Antonio Riotto

Publication date: 4 January 2006

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0507573

zbMATH Keywords

inflationcosmologycosmological perturbations

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (2)

Effects of quantum gravity on the inflationary parameters and thermodynamics of the early universe ⋮ Ricci reheating

Cites Work

• The cosmology of string theoretic axions
• de Sitter vacua in string theory
• Scales and hierarchies in warped compactifications and brane worlds

This page was built for publication: POST-INFLATION INCREASE OF THE COSMOLOGICAL TENSOR-TO-SCALAR PERTURBATION RATIO