ANGULAR POWER SPECTRUM IN MODULAR INVARIANT INFLATION MODEL

DOI10.1142/S0217751X07036440zbMath1117.83126arXivastro-ph/0609657OpenAlexW2601815446MaRDI QIDQ5293952

Mitsuo J. Hayashi, Kenji Takagi, Tomoki Watanabe, Tomoyuki Takami, Shiro Hirai, Yusuke Okamei

Publication date: 5 July 2007

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

Full work available at URL: https://arxiv.org/abs/astro-ph/0609657

zbMATH Keywords

inflationmodular invariant potentialWMAP observations

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Astrophysical cosmology (85A40)

Related Items (1)

INFLATION AND ACCELERATING UNIVERSE IN MODIFIED MODULAR INVARIANT SUPERGRAVITY

Cites Work

• \(N=1\) no-scale supergravity from IIB orientifolds
• Cosmological Inflation and Large-Scale Structure
• Effect of the length of inflation on angular TT and TE power spectra in power-law inflation
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

This page was built for publication: ANGULAR POWER SPECTRUM IN MODULAR INVARIANT INFLATION MODEL