MSSM Dark Matter in Light of Higgs and LUX Results

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...

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Main Authors: W. Abdallah, S. Khalil
Format: Article
Language:English
Published: Hindawi Limited 2016-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2016/5687463
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spelling doaj-0fe36513d275479094947339785594e42020-11-24T22:54:20ZengHindawi LimitedAdvances in High Energy Physics1687-73571687-73652016-01-01201610.1155/2016/56874635687463MSSM Dark Matter in Light of Higgs and LUX ResultsW. Abdallah0S. Khalil1Center for Fundamental Physics, Zewail City of Science and Technology, 6th of October City, Giza 12588, EgyptCenter for Fundamental Physics, Zewail City of Science and Technology, 6th of October City, Giza 12588, EgyptThe 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 tan⁡β  (~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: m0≃O(4) TeV and m1/2≃600 GeV for low tan⁡β  (~10); m0~m1/2≃O(1) TeV or m0≃O(4) TeV and m1/2≃700 GeV for large tan⁡β  (~50).http://dx.doi.org/10.1155/2016/5687463
collection DOAJ
language English
format Article
sources DOAJ
author W. Abdallah
S. Khalil
spellingShingle W. Abdallah
S. Khalil
MSSM Dark Matter in Light of Higgs and LUX Results
Advances in High Energy Physics
author_facet W. Abdallah
S. Khalil
author_sort W. Abdallah
title MSSM Dark Matter in Light of Higgs and LUX Results
title_short MSSM Dark Matter in Light of Higgs and LUX Results
title_full MSSM Dark Matter in Light of Higgs and LUX Results
title_fullStr MSSM Dark Matter in Light of Higgs and LUX Results
title_full_unstemmed MSSM Dark Matter in Light of Higgs and LUX Results
title_sort mssm dark matter in light of higgs and lux results
publisher Hindawi Limited
series Advances in High Energy Physics
issn 1687-7357
1687-7365
publishDate 2016-01-01
description 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 tan⁡β  (~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: m0≃O(4) TeV and m1/2≃600 GeV for low tan⁡β  (~10); m0~m1/2≃O(1) TeV or m0≃O(4) TeV and m1/2≃700 GeV for large tan⁡β  (~50).
url http://dx.doi.org/10.1155/2016/5687463
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AT skhalil mssmdarkmatterinlightofhiggsandluxresults
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