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arXiv · 0912.2324

Low-scale Inflation and Supersymmetry Breaking in Racetrack Models

Rouzbeh Allahverdi·Bhaskar Dutta·Kuver Sinha
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Abstract

In many moduli stabilization schemes in string theory, the scale of inflation appears to be of the same order as the scale of supersymmetry breaking. For low-scale supersymmetry breaking, therefore, the scale of inflation should also be low, unless this correlation is avoided in specific models. We explore such a low-scale inflationary scenario in a racetrack model with a single modulus in type IIB string theory. Inflation occurs near a point of inflection in the Kähler modulus potential. Obtaining acceptable cosmological density perturbations leads to the introduction of magnetized D7-branes sourcing non-perturbative superpotentials. The gravitino mass, m_{3/2}, is chosen to be around 30 TeV, so that gravitinos that are produced in the inflaton decay do not affect big-bang nucleosynthesis. Supersymmetry is communicated to the visible sector by a mixture of anomaly and modulus mediation. We find that the two sources contribute equally to the gaugino masses, while scalar masses are decided mainly by anomaly contribution. This happens as a result of the low scale of inflation and can be probed at the LHC.

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Rouzbeh Allahverdi, Bhaskar Dutta, Kuver Sinha. 2009-12-11. Low-scale Inflation and Supersymmetry Breaking in Racetrack Models. https://doi.org/10.1103/physrevd.81.083538

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