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Kadota, Kenji; Kobayashi, Tatsuo; Oikawa, Akane; Omoto, Naoya; Otsuka, Hajime; Tatsuishi, Takuya H.
Funding organisation: SCOAP3, CERN, Geneva (Switzerland)2016
Funding organisation: SCOAP3, CERN, Geneva (Switzerland)2016
AbstractAbstract
[en] 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.
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Available from http://dx.doi.org/10.1088/1475-7516/2016/10/013; Available from http://repo.scoap3.org/record/17556; PUBLISHER-ID: JCAP10(2016)013; OAI: oai:repo.scoap3.org:17556; cc-by Article funded by SCOAP3. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 License. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.; Country of input: International Atomic Energy Agency (IAEA)
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Journal Article
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Journal of Cosmology and Astroparticle Physics; ISSN 1475-7516;
; v. 2016(10); p. 13

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