Swampland, Trans-Planckian Censorship and Fine-Tuning Problem for Inflation: Tunnelling Wavefunction to the Rescue
arXiv:2002.02941 · doi:10.1088/1475-7516/2020/10/037
Abstract
The trans-Planckian censorship conjecture implies that single-field models of inflation require an extreme fine-tuning of the initial conditions due to the very low-scale of inflation. In this work, we show how a quantum cosmological proposal -- namely the tunneling wavefunction -- naturally provides the necessary initial conditions without requiring such fine-tunings. More generally, we show how the tunneling wavefunction can provide suitable initial conditions for hilltop inflation models, the latter being typically preferred by the swampland constraints.
14 pages, comments welcome; v2: references added
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Cited by in corpus (13)
- Reheating in small-field inflation on the brane: The Swampland Criteria and observational constraints in light of the PLANCK 2018 results
- Swampland Conjecture and Inflation Model from Brane Perspective
- Brane inflation and Trans-Planckian censorship conjecture
- Einselection, Equilibrium and Cosmology
- Dynamically Generated Inflationary Lambda-CDM
- Generation of inflationary perturbations in the continuous spontaneous localization model: The second order power spectrum
- Note on initial conditions for small-field inflation
- A Local Wheeler-DeWitt Measure for the String Landscape
- Multi-field inflation from single-field models
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- Escape from the swamp with spectator
- Fuzzy instantons in landscape and swampland: review of the Hartle-Hawking wave function and several applications
- Wave function of the universe in the presence of trans-Planckian censorship