De Sitter vs Quintessence in String Theory
Aug 27, 2018
49 pages
Published in:
- Fortsch.Phys. 67 (2019) 1-2, 1800079
- Published: Jan 1, 2019
e-Print:
- 1808.08967 [hep-th]
DOI:
- 10.1002/prop.201800079 (publication)
View in:
Citations per year
Abstract: (WILEY)
De Sitter solutions have been recently conjectured to be incompatible with quantum gravity. In this paper we critically assess the progress and challenges of different mechanisms to obtain de Sitter vacua in string compactifications and compare them to quintessence models. We argue that, despite recent criticisms, de Sitter models reached a level of concreteness and calculational control which has been improving over time. On the other hand, building string models of quintessence appears to be more challenging and requires additional fine‐tuning. We discuss the tension between the swampland conjecture and the Higgs potential and find examples which can evade fifth‐force bounds even if they seem very hard to realise in string theory. We also comment on the tension with low‐redshift data and explore ultra‐light axions from string theory as dark energy candidates.Note:
- Published in Fortschritte der Physik
- de Sitter
- quintessence
- swampland
- string Landscape
- vacuum state: de Sitter
- string: compactification
- potential: Higgs
- string model
- quintessence
- tension
References(184)
Figures(4)
- [1]
- [2]
- [3]
- [4]
- [5]
- [6]
- [7]
- [8]
- [9]
- [10]
- [11]
- [12]
- [13]
- [14]
- [15]
- [16]
- [17]
- [18]
- [19]
- [20]
- [21]
- [22]
- [23]
- [24]
- [25]