arXiv:1404.1680·v3·Cosmology and Nongalactic Astrophysics
Topological Inflation with Large Tensor-to-scalar Ratio
Yu-Chieh Chung🇯🇵 · Chunshan Lin🇯🇵
Abstract
BICEP2's detection on the primordial B-mode of CMB polarization suggests that inflation occurred around GUT scale, with the tensor-to-scalar ratio r~0.2. Inspired by this discosvery, we study the topological inflation which was driven by a double/single/no well potential. We show that with proper choice of parameters, all these three types of topological inflationary models could be consistent with the constraints from current observations.
Comments: 5 pages, 6 figures, PRD format; v2 typos corrected, references added