Multi-field cold and warm inflation and the de Sitter swampland conjectures
arXiv:2204.13794 · doi:10.1088/1475-7516/2022/09/001
Abstract
We discuss under which conditions multi-field cold and warm inflationary models with canonical kinetic energy terms are compatible with the swampland conjectures about the emergence of de Sitter solutions in string theory. We find that under quite general conditions the slow-roll conditions for multi-field cold inflation are at odds with the swampland conjectures for an arbitrary number of scalar fields driving inflation. However, slow-roll conditions can be reconciled with the swampland conjectures in the strong dissipative regime of warm inflation.
15 pages, extended discussion and references included
References in corpus (7)
- On the Geometry of the String Landscape and the Swampland
- The Swampland: Introduction and Review
- Triple unification of inflation, dark energy, and dark matter in two-scalar-field cosmology
- Quintessence and the Swampland: The parametrically controlled regime of moduli space
- Unification of inflation, dark energy, and dark matter within the Salam-Sezgin cosmological model
- Inflation, phase transitions and the cosmological constant
- String-Inspired Running Vacuum, the "Vacuumon", and the Swampland Criteria