Strong Planck constraints on braneworld and non-commutative inflation

Gianluca Calcagni, Sachiko Kuroyanagi, Junko Ohashi, Shinji Tsujikawa

研究成果: Article査読

24 被引用数 (Scopus)

抄録

We place observational likelihood constraints on braneworld and non-commutative inflation for a number of inflaton potentials, using Planck, WMAP polarization and BAO data. Both braneworld and non-commutative scenarios of the kind considered here are limited by the most recent data even more severely than standard general-relativity models. At more than 95 % confidence level, the monomial potential V(φ)φp is ruled out for p 2 in the Randall-Sundrum (RS) braneworld cosmology and, for p > 0, also in the high-curvature limit of the Gauss-Bonnet (GB) braneworld and in the infrared limit of non-commutative inflation, due to a large scalar spectral index. Some parameter values for natural inflation, small-varying inflaton models and Starobinsky inflation are allowed in all scenarios, although some tuning is required for natural inflation in a non-commutative spacetime.

本文言語English
論文番号052
ジャーナルJournal of Cosmology and Astroparticle Physics
2014
3
DOI
出版ステータスPublished - 2014 3
外部発表はい

ASJC Scopus subject areas

  • 天文学と天体物理学

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