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XENON100 Implications for Naturalness in the MSSM, NMSSM and lambda-SUSY · Around

2012

XENON100 Implications for Naturalness in the MSSM, NMSSM and lambda-SUSY

Perelstein, Maxim, Shakya, Bibhushan

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In a recent paper arXiv:1107.5048, we discussed the correlation between the elastic neutralino-nucleon scattering cross section, constrained by dark matter direct detection experiments, and fine-tuning at tree-level in the electroweak symmetry breaking sector of the Minimal Supersymmetric Standard Model (MSSM).

Here, we show that the correlation persists in the Next-to-Minimal Supersymmetric Standard Model (NMSSM), and its variant, lambda-SUSY.
Both models are strongly motivated by the recent discovery of a 125 GeV Higgs-like particle.
We also discuss the implications of the recently published bound on the direct detection cross section from 225 live days of XENON100 experiment.

Built on

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For reviews, see for example G. Jungman, M. Kamionkowski and K. Griest, “Supersymmetric dark matter,”
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Then

M. Perelstein and B. Shakya, “Fine-Tuning Implications of Direct Dark Matter Searches in the MSSM,”
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2011
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J. L. Feng and D. Sanford, “Heart of Darkness: The Significance of the Zeptobarn Scale for Neutralino Direct Detection,”
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U. Ellwanger, G. Espitalier-Noel and C. Hugonie, “Naturalness and Fine Tuning in the NMSSM: Implications of Early LHC Results,”
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A. V. Belikov, J. F. Gunion, D. Hooper and T. M. P. Tait, “CoGeNT, DAMA, and Light Neutralino Dark Matter,” Phys. Lett. B 705
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2011
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R. Kappl, M. Ratz and M. W. Winkler, “Light dark matter in the singlet-extended MSSM,” Phys. Lett. B 695

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