| Article | |
| Report number | arXiv:1209.0499 ; CERN-PH-TH-2012-228 ; CPHT-RR069.0812 ; UMN-TH-3116-12 ; LPT-ORSAY-12-92 ; UH-511-1199-12 ; FTPI-MINN-12-28 ; CERN-PH-TH-2012-228 ; CPHT-RR069.0812 ; UMN-TH-3116-12 ; FTPI-MINN-12-28 ; LPT-ORSAY-12-92 ; UH-511-1199-12 |
| Title | Strong moduli stabilization and phenomenology |
| Author(s) | Dudas, Emilian (Orsay, LPT ; Ecole Polytechnique, CPHT ; CERN) ; Linde, Andrei (Stanford U., Phys. Dept. ; Stanford U., ITP) ; Mambrini, Yann (Orsay, LPT) ; Mustafayev, Azar (Hawaii U. ; Minnesota U., Theor. Phys. Inst.) ; Olive, Keith A. (Minnesota U., Theor. Phys. Inst.) |
| Publication | 2013-01-15 |
| Imprint | 05 Sep 2012 |
| Number of pages | 21 |
| Note | Comments: 21 pages, 7 figures 21 pages, 7 figures, final version with updated Figures 2 and 3 |
| In: | Eur. Phys. J. C 73 (2013) 2268 |
| DOI | 10.1140/epjc/s10052-012-2268-7 |
| Subject category | Particle Physics - Phenomenology |
| Abstract | We describe the resulting phenomenology of string theory/supergravity models with strong moduli stabilization. The KL model with F-term uplifting, is one such example. Models of this type predict universal scalar masses equal to the gravitino mass. In contrast, A-terms receive highly suppressed gravity mediated contributions. Under certain conditions, the same conclusion is valid for gaugino masses, which like A-terms, are then determined by anomalies. In such models, we are forced to relatively large gravitino masses (30-1000 TeV). We compute the low energy spectrum as a function of m_{3/2}. We see that the Higgs masses naturally takes values between 125-130 GeV. The lower limit is obtained from the requirement of chargino masses greater than 104 GeV, while the upper limit is determined by the relic density of dark matter (wino-like). |
| Copyright/License | Preprint: © 2012-2025 CERN (License: CC-BY-3.0) |
Corresponding record in: Inspire
Záznam vytvorený 2012-09-05, zmenený 2023-03-14
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