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2019
DOI: 10.1007/jhep11(2019)134
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The F -term problem and other challenges of stringy quintessence

Abstract: We attempt a systematic analysis of string-theoretic quintessence models as an alternative to metastable de Sitter vacua. It appears that, within the boundaries of what is known, largevolume type-IIB flux compactifications are preferred. Here the quintessence scalar is the ratio of certain 4-cycle volumes. It has already been noticed that the volume modulus, which must be stabilized, tends to remain too light. One may call this the "light volume problem". In addition, we identify an "F -term problem": The posi… Show more

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Cited by 36 publications
(36 citation statements)
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“…This limits the applicability to practical questions, where some of the 'large' quantities 22 The path towards a realistic string phenomenology relying on quintessence instead of de Sitter has serious issues of its own, at least in the better-understood part of the landscape. [80] are really not that large (cf. our M ≳ 12).…”
Section: Appendix: Comment On the Numerical Prefactorsmentioning
confidence: 99%
“…This limits the applicability to practical questions, where some of the 'large' quantities 22 The path towards a realistic string phenomenology relying on quintessence instead of de Sitter has serious issues of its own, at least in the better-understood part of the landscape. [80] are really not that large (cf. our M ≳ 12).…”
Section: Appendix: Comment On the Numerical Prefactorsmentioning
confidence: 99%
“…In any case, a no-dS viewpoint leads one to naturally focus on runaway potentials [25] in string theory and to quintessence models in phenomenology [26,27] (see [28] for a review). Embedding quintessence in string theory is also difficult and we will not go into any detail of this, but instead refer to [29][30][31].…”
Section: Jhep05(2020)114mentioning
confidence: 99%
“…[1,2,3] 1 . Therefore the quintessence type of dark energy [7,8,9,10], that can be provided by runaway potentials, deserves a detailed study both in supergravity and in string theory [11,12,13,14,15,16,17,18,19,20,21,22]. In this contribution we will study quintessence from the perspective of a pure gravitational theory, we will show how such dynamics can naturally arise, and we will in particular embed these models in four-dimensional N=1 supergravity.…”
Section: Introduction and Discussionmentioning
confidence: 99%