A new class of de Sitter vacua in type IIB large volume compactifications

被引:44
作者
Gallego, Diego [1 ]
Marsh, M. C. David [2 ]
Vercnocke, Bert [3 ]
Wrase, Timm [4 ]
机构
[1] UPTC, Escuela Fis, Ave Cent Norte, Tunja, Colombia
[2] Univ Cambridge, Dept Appl Math & Theoret Phys, Wilberforce Rd, Cambridge CB3 0WA, England
[3] Katholieke Univ Leuven, Inst Theoret Phys, Celestijnenlaan 200D, B-3001 Leuven, Belgium
[4] TU Wien, Inst Theoret Phys, Wiedner Hauptstr 8-10, A-1040 Vienna, Austria
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2017年 / 10期
基金
奥地利科学基金会; 欧洲研究理事会; 美国国家科学基金会;
关键词
Flux compactifications; Supergravity Models; Superstring Vacua; COSMOLOGICAL IMPLICATIONS; SUPERSYMMETRY BREAKING; SOFT TERMS; SUPERGRAVITY;
D O I
10.1007/JHEP10(2017)193
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We construct a new class of metastable de Sitter vacua of flux compactifications of type IIB string theory. These solutions provide a natural extension of the 'Large Volume Scenario' anti-de Sitter vacua, and can analogously be realised at parametrically large volume and weak string coupling, using standard N = 1 supergravity. For these new vacua, a positive vacuum energy is achieved from the inclusion of a small amount of flux-induced supersymmetry breaking in the complex structure and axio-dilaton sector, and no additional 'uplift' contribution (e.g. from anti-branes) is required. We show that the approximate no-scale structure of the effective theory strongly influences the spectrum of the stabilised moduli: one complex structure modulus remains significantly lighter than the supersymmetry breaking scale, and metastability requires only modest amounts of tuning. After discussing these general results, we provide a recipe for constructing de Sitter vacua on a given compactification manifold, and give an explicit example of a de Sitter vacuum for the compactification on the Calabi-Yau orientifold realised in CP111694. Finally, we note that these solutions have intriguing implications for phenomenology, predicting no superpartners in the spectrum below similar to 50 TeV, and no WIMP dark matter.
引用
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页数:34
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