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).
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Notes
In most of the formulas of this letter, M P =1. In some formulas, however, we keep explicitly M P .
If we allow a coupling of the form \(h_{A} = h_{A}^{0} (1 + \beta_{A} e^{-2aT} S)\), we would find a suppression \(m_{1/2} \propto m_{3/2}^{2}/M_{P}\).
A posteriori, we know that for very small A 0/m 0 the requirement for relatively large Higgs masses would lead to the same conclusion regarding large scalar masses, which to control the relic density would also require anomaly mediation for gaugino masses.
The GUT scale, M GUT, is defined as the scale where SU(2) and U(1) gauge couplings unify and is approximately 1.5×1016 GeV.
Note that the upper limit on m 0 can be raised significantly for small λ and large A 0/m 0. Of course in the KL models discussed here, A 0/m 0 is very small.
We note that there is at least a 2–3 GeV uncertainty in the Higgs mass calculation, so that we cannot out of hand exclude results with Higgs masses at 130 GeV.
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Acknowledgements
We are very grateful to M. Arvanitaki, S. Dimopoulos, T. Gherghetta, P. Graham, R. Kallosh, J. March-Russell and X. Tata for many interesting discussions and suggestions. The work of E.D. was supported in part by the ERC Advanced Investigator Grant No. 226371 “Mass Hierarchy and Particle Physics at the TeV Scale” (MassTeV) and by the contract PITN-GA-2009-237920. The work of E.D. and Y.M. was supported in part by the French ANR TAPDMS ANR-09-JCJC-0146. The work by A.L. was supported by NSF grant PHY-0756174 at Stanford University. The work of A.M. and K.A.O. is supported in part by DOE grant DE-FG02-94ER-40823 at the University of Minnesota. The work of A.M. is also supported in part by DOE grant DE-FG02-04ER-41291 at the University of Hawaii.
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Dudas, E., Linde, A., Mambrini, Y. et al. Strong moduli stabilization and phenomenology. Eur. Phys. J. C 73, 2268 (2013). https://doi.org/10.1140/epjc/s10052-012-2268-7
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DOI: https://doi.org/10.1140/epjc/s10052-012-2268-7