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Then

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2013

Electroweak Supersymmetry (EWSUSY) in the NMSSM

Cheng, Taoli, Li, Tianjun

Understand

To explain all the available experimental results, we have proposed the Electroweak Supersymmetry (EWSUSY) previously, where the squarks and/or gluino are heavy around a few TeVs while the sleptons, sneutrinos, Bino, Winos, and/or Higgsinos are light within one TeV.

In the Next to Minimal Supersymmetric Standard Model (NMSSM), we perform the systematic \chi^2 analyses on parameter space scan for three EWSUSY scenarios: (I) R-parity conservation and one dark matter candidate; (II) R-parity conservation and multi-component dark matter; (III) R-parity violation.
We obtain the minimal \chi^2/(degree of freedom) of 10.2/15, 9.6/14, and 9.2/14 respectively for Scenarios I, II, and III.
Considering the constraints from the LHC neutralino/chargino and slepton searches, we find that the majority of viable parameter space prefered by the muon anomalous magnetic moment has been excluded except for the parameter space with moderate to large \tan\beta (\ge 8).

Built on

T. Moroi, Phys. Rev. D 53
1997
Earlier work this paper cites.
S. Y. Choi, D. J. Miller, and P. M. Zerwas, Nucl. Phys. B 711
1999
Earlier work this paper cites.
S. P. Martin and J. D. Wells, Phys. Rev. D 64
2001
Earlier work this paper cites.
M. Byrne, C. Kolda and J. E. Lennon, Phys. Rev. D 67
2003
Earlier work this paper cites.
U. Ellwanger, J. F. Gunion and C. Hugonie, JHEP 0502
2005
Earlier work this paper cites.
G. Belanger, F. Boudjema, A. Pukhov and A. Semenov, Comput. Phys. Commun. 174
2006
Earlier work this paper cites.
T. Sjostrand, S. Mrenna and P. Z. Skands, JHEP 0605
2006
Earlier work this paper cites.
D. Stockinger, J. Phys. G 34
2007
Earlier work this paper cites.
B. C. Allanach, M. A. Bernhardt, H. K. Dreiner, C. H. Kom and P. Richardson, Phys. Rev. D 75
2007
Earlier work this paper cites.
A. Djouadi, Phys. Rept. 459
2008
Earlier work this paper cites.
F. Domingo and U. Ellwanger, JHEP 0807
Original
2008
Earlier work this paper cites.
O. Buchmueller, R. Cavanaugh, A. De Roeck, J. R. Ellis, H. Flacher, S. Heinemeyer, G. Isidori and K. A. Olive et al
Original
2009
Earlier work this paper cites.