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.
arXiv comment7 pages, References added
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- A Note on Noncommutative Brane Inflation
- Noncommutative KKLMMT Model
- Inflation and the semiclassical dynamics of a conformal scalar field
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