Thermal, Trapped and Chromo-Natural Inflation in light of the Swampland Criteria and the Trans-Planckian Censorship Conjecture
arXiv:2006.01902 · doi:10.1140/epjc/s10052-021-09240-3
Abstract
We consider thermal, trapped and chromo-natural inflation in light of the swampland criteria and the Trans-Planckian Censorship Conjecture (TCC). Since thermal inflation occurs at energies low compared to those of Grand Unification, it is consistent with the TCC, and it is also consistent with the refined swampland conditions. Trapped and chromo-natural inflation are candidates for primordial (high energy scale) inflation. Since in both of these scenarios there are effective damping terms in the scalar field equation of motion, the models can easily be consistent with the swampland criteria. The TCC, on the other hand, constrains these scenarios to only take place at low energies.
arXiv comment8 pages
References in corpus (54)
- Towards the Theory of Reheating After Inflation
- Reheating after Inflation
- On the Geometry of the String Landscape and the Swampland
- Universe Reheating after Inflation
- The Swampland: Introduction and Review
- Warm Inflation
- Distance and de Sitter Conjectures on the Swampland
- Reheating in Inflationary Cosmology: Theory and Applications
- On the Cosmological Implications of the String Swampland
- Nonperturbative Dynamics Of Reheating After Inflation: A Review
- Thermal Inflation and the Moduli Problem
- Bounds on Slow Roll and the de Sitter Swampland
- De Sitter Space and the Swampland
- Gauge Fields and Inflation
- The Best Inflationary Models After Planck
- Chromo-Natural Inflation: Natural inflation on a steep potential with classical non-Abelian gauge fields
- Beauty is Attractive: Moduli Trapping at Enhanced Symmetry Points
- Probing Planckian physics: resonant production of particles during inflation and features in the primordial power spectrum
- Trans-Planckian Censorship and Inflationary Cosmology
- Non-Abelian Gauge Field Inflation
- Warm Little Inflaton
- Inflationary Constraints on Type IIA String Theory
- The importance of being warm (during inflation)
- The string swampland constraints require multi-field inflation
- A First Principles Warm Inflation Model that Solves the Cosmological Horizon/Flatness Problems
- Quantum Break-Time of de Sitter
- Dark Energy in the Swampland
- Warm inflation as a way out of the swampland
- Trapped Inflation
- On Exclusion of Positive Cosmological Constant
- Moduli Stabilization with the String Higgs Effect
- Warm Inflation in the light of Swampland Criteria
- Supersymmetry Breaking by Fluxes
- Constraining de Sitter Space in String Theory
- Quantum Breaking Bound on de Sitter and Swampland
- Initial Conditions for Inflation - A Short Review
- Swampland Distance Conjecture, Inflation and -attractors
- Distance, de Sitter and Trans-Planckian Censorship conjectures: the status quo of Warm Inflation
- Universal Upper Bound on the Inflationary Energy Scale from the Trans-Planckian Censorship Conjecture
- Quantum Corrections and the de Sitter Swampland Conjecture
- The Ubiquitous Inflaton in String-Inspired Models
- Trans-Planckian censorship and other swampland bothers addressed in warm inflation
- Trans-Planckian censorship of multistage inflation and dark energy
- Trans-Planckian Censorship Conjecture and Non-thermal post-inflationary history
- Pre-inflation and Trans-Planckian Censorship
- Strengthening the TCC Bound on Inflationary Cosmology
- Relaxing the TCC Bound on Inflationary Cosmology?
- Obstacles to Constructing de Sitter Space in String Theory
- Role of trans-Planckian modes in cosmology
- Non-Standard Cosmological Models and the trans-Planckian Censorship Conjecture
- Inflation and Decoupling
- Reheating After Swampland Conjecture
- String Gases and the Swampland
- Note on Shape Moduli Stabilization, String Gas Cosmology and the Swampland Criteria