Helical Inflation and Cosmic Strings
  Recent BICEP2 detection of low-multipole B-mode polarization anisotropy in
the cosmic microwave background radiation supports the inflationary universe
scenario and suggests a large inflaton field range. The latter feature can be
achieved with axion fields in the framework of string theory. We present such a
helical model which naturally becomes a model with a single cosine potential,
and which in turn reduces to the (quadratic) chaotic inflation model in the
super-Planckian limit. The slightly smaller tensor/scalar ratio $r$ of models
of this type provides a signature of the periodic nature of an axion potential.
We present a simple way to quantify this distinctive feature. As axions are
intimately related to strings/vortices and strings are ubiquitous in string
theory, we explore the possibility that cosmic strings may be contributing to
the B-mode polarization anisotropy observed.
