arXiv · 1412.2724
Spiral Inflation
Abstract
We propose a novel scenario of primordial inflation in which the inflaton goes through a spiral motion starting from around the top of a symmetry breaking potential. We show that, even though inflation takes place for a field value much smaller than Planck scale, it is possible to obtain relatively large tensor to scalar ratio ($r \sim 0.1$) without fine tuning. The inflationary observables perfectly match Planck data.
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Gabriela Barenboim, Wan-Il Park. 2015-01-21. Spiral Inflation. https://doi.org/10.1016/j.physletb.2014.12.042
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