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Advances in High Energy Physics
Volume 2016, Article ID 5687463, 10 pages
Research Article

MSSM Dark Matter in Light of Higgs and LUX Results

1Center for Fundamental Physics, Zewail City of Science and Technology, 6th of October City, Giza 12588, Egypt
2Department of Mathematics, Faculty of Science, Cairo University, Giza 12613, Egypt

Received 26 September 2015; Accepted 6 December 2015

Academic Editor: Enrico Lunghi

Copyright © 2016 W. Abdallah and S. Khalil. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. The publication of this article was funded by SCOAP3.


The constraints imposed on the Minimal Supersymmetric Standard Model (MSSM) parameter space by the Large Hadron Collider (LHC) Higgs mass limit and gluino mass lower bound are revisited. We also analyze the thermal relic abundance of lightest neutralino, which is the Lightest Supersymmetric Particle (LSP). We show that the combined LHC and relic abundance constraints rule out most of the MSSM parameter space except a very narrow region with very large   (~50). Within this region, we emphasize that the spin-independent scattering cross section of the LSP with a proton is less than the latest Large Underground Xenon (LUX) limit by at least two orders of magnitude. Finally, we argue that nonthermal Dark Matter (DM) scenario may relax the constraints imposed on the MSSM parameter space. Namely, the following regions are obtained:  TeV and  GeV for low   (~10);  TeV or  TeV and  GeV for large   (~50).