The Swampland Conjectures and Slow-Roll Thawing Quintessence
arXiv:2008.05465 · doi:10.1103/PhysRevD.102.063519
Abstract
We examine the Swampland conjectures in the context of generic slow-roll thawing quintessence models. Defining and , where is the initial value of , we find regions of parameter space consistent with both observational data and with the refined de Sitter conjecture, and we show that all such models satisfy the distance conjecture. We quantify the degree of fine-tuning on needed to achieve these results.
8 pages, 5 figures, references added
References in corpus (11)
- Dynamics of dark energy
- The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
- Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
- Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation
- On the Geometry of the String Landscape and the Swampland
- Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
- Thawing quintessence with a nearly flat potential
- Hilltop Quintessence
- Swampland Conjectures and Late-Time Cosmology
- Dark energy beyond quintessence: Constraints from the swampland
- Dark Energy, Extra Dimensions, and the Swampland