A general condition of inflationary cosmology on trans-Planckian physics
arXiv:hep-th/0312013 · doi:10.1142/S0217751X05021178
Abstract
We consider a more general initial condition satisfying the minimal uncertainty relationship. We calculate the power spectrum of a simple model in inflationary cosmology. The results depend on perturbations generated below a fundamental scale, e.g. the Planck scale.
7 pages, References added