Detailed investigation of the duration of inflation in loop quantum
  cosmology for a Bianchi-I universe with different inflaton potentials and
  initial conditions
  There is a wide consensus on the correct dynamics of the background in loop
quantum cosmology. In this article we make a systematic investigation of the
duration of inflation by varying what we think to be the most important
"unknowns" of the model: the way to set initial conditions, the amount of shear
at the bounce and the shape of the inflaton potential.
