Constraints on Dark Energy from Inflation and the Swampland Conjectures
arXiv:1911.00925
Abstract
We discuss the prospects of measuring deviations of the dark energy equation of state from w=-1 by using the swampland conjectures to relate inflationary models to quintessence scenarios. This note is based on work done by the author with H. Murayama and C. Chiang arXiv:1811.01987.
arXiv comment7 Pages, contribution to proceedings for Rencontres du Vietnam "Cosmology", August 2019 v2: Added References
References in corpus (12)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- On the Geometry of the String Landscape and the Swampland
- Symmetries and Strings in Field Theory and Gravity
- On the Cosmological Implications of the String Swampland
- The String Landscape and the Swampland
- The landscape, the swampland and the era of precision cosmology
- Sound Speed of Primordial Fluctuations in Supergravity Inflation
- The dS swampland conjecture with the electroweak symmetry and QCD chiral symmetry breaking
- Phenomenological Consequences of the Refined Swampland Conjecture
- What does Inflation say about Dark Energy given the Swampland Conjectures?
- From Swampland to Phenomenology and Back