Shaft Inflation and the Planck satellite observations
  A new family of inflation models is introduced and studied. The models are
characterised by a scalar potential which, far from the origin, approaches an
inflationary plateau in a power-law manner, while near the origin becomes
monomial, as in chaotic inflation. The models are obtained in the context of
global supersymmetry starting with a superpotential, which interpolates from a
generalised monomial to an O'Raifearteagh form for small to large values of the
inflaton field respectively. It is demonstrated that the observables obtained,
such as the scalar spectral index, its running and the tensor to scalar ratio,
are in excellent agreement with the latest observations, without any
fine-tuning. Moreover, by widening mildly the shaft in field space, it is shown
that sizable tensors can be generated, which may well be observable in the near
future.
