  We present a simple two-field model of inflation and show how to embed it in
string theory as a straightforward generalization of axion monodromy models.
Phenomenologically, the predictions are equivalent to those of chaotic
inflation, and in particular include observably large tensor modes. The whole
high-scale large-field inflationary dynamics takes place within a region of
field space that is parametrically subplanckian in diameter, hence improving
our ability to control quantum corrections and achieve slow-roll inflation.
