  In this paper, we discuss the properties of one-parameter sequences that
arise when solving the Hamiltonian constraint in Bianchi I loop quantum
cosmology using a separation of variables method. In particular, we focus on
finding an expression for the sequence for all real values of the parameter,
and discuss the pre-classicality of this function. We find that the behavior of
these preclassical sequences imply time asymmetry on either side of the
classical singularity in Bianchi I cosmology.
