Small field axion inflation with sub-Planckian decay constant

Kenji Kadota, Tatsuo Kobayashi, Akane Oikawa, Naoya Omoto, Hajime Otsuka, Takuya H. Tatsuishi

    研究成果: Article

    6 引用 (Scopus)

    抜粋

    We study an axion inflation model recently proposed within the framework of type IIB superstring theory, where we pay a particular attention to a sub-Planckian axion decay constant. Our axion potential can lead to the small field inflation with a small tensor-to-scalar ratio, and a typical reheating temperature can be as low as GeV.

    元の言語English
    記事番号013
    ジャーナルJournal of Cosmology and Astroparticle Physics
    2016
    発行部数10
    DOI
    出版物ステータスPublished - 2016 10 10

    ASJC Scopus subject areas

    • Astronomy and Astrophysics

    フィンガープリント Small field axion inflation with sub-Planckian decay constant' の研究トピックを掘り下げます。これらはともに一意のフィンガープリントを構成します。

  • これを引用

    Kadota, K., Kobayashi, T., Oikawa, A., Omoto, N., Otsuka, H., & Tatsuishi, T. H. (2016). Small field axion inflation with sub-Planckian decay constant. Journal of Cosmology and Astroparticle Physics, 2016(10), [013]. https://doi.org/10.1088/1475-7516/2016/10/013