Abstract
We show that if the α-attractor model is realized by the spontaneous breaking of the scale symmetry, then the stability and the dynamics of the vector field that gauges the scale symmetry can severely constrain the α-parameter as 5 / 6 < α< 1 restricting the inflationary predictions in a very tiny region in the ns- r plane that are in great agreement with the latest Planck data. Although the different values of α do not make a tangible difference for ns and r, they provide radically different scenarios for the post-inflationary dynamics which determines the standard BBN processes and the large scale isotropy of the universe.
Original language | English |
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Article number | 306 |
Journal | European Physical Journal C |
Volume | 77 |
Issue number | 5 |
DOIs | |
Publication status | Published - 1 May 2017 |
Bibliographical note
Publisher Copyright:© 2017, The Author(s).
Funding
We thank Gokhan Alkac, Glenn Barnich and Shahin Sheikh-Jabbari for valuable comments on conserved charges, and Renata Kallosh, Andrei Linde, Diederik Roest and Marco Scalisi for valuable comments on superconformal -attractors. ÖA acknowledges the support by the Distinguished Young Scientist Award BAGEP of the Science Academy. EOK acknowledges the support by Turkish Academy of Sciences Distinguished Young Scientist Award TÜBA-GEBİP 2015. The work of MO is supported in part by the Marie Curie Cofund (No. 116C028).
Funders | Funder number |
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Marie Curie Cofund | 116C028 |
Türkiye Bilimler Akademisi | |
Bilim Akademisi |