Trans-Planckian censorship of multistage inflation and dark energy
arXiv:1911.06148 · doi:10.1103/PhysRevD.101.063527
Abstract
We explore the bound of the trans-Planckian censorship conjecture on an inflation model with multiple stages. We show that if the first inflationary stage is responsible for the primordial perturbations in the cosmic microwave background window, the -folding number of each subsequent stage will be bounded by the energy scale of the first stage. This seems to imply that the lifetime of the current era of accelerated expansion (regarded as one of the multiple inflationary stages) might be a probe for distinguishing inflation from its alternatives. We also present a multistage inflation model in a landscape consisting of anti-de Sitter vacua separated by potential barriers.
13 pages, 4 figures; references added; updated to match published version
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- Limitations of an Effective Field Theory Treatment of Early Universe Cosmology
- Populating the landscape in an inhomogeneous universe
- Large against Trans-Planckian Censorship in Scalar-Tensor Theory?
- Escape from the swamp with spectator
- Trans-Planckian Censorship Conjecture and Early Universe Cosmology
- Implications of single field inflation in general cosmological scenarios on the nature of dark energy given the swampland conjectures