Constrained SUSY seesaws with a 125 GeV Higgs

被引:0
作者
M. Hirsch
F. R. Joaquim
A. Vicente
机构
[1] AHEP Group,Departamento de Física and Centro de Física Teórica de Partículas, Instituto Superior Técnico
[2] Instituto de Física Corpuscular — C.S.I.C./Universitat de València,undefined
[3] Edificio de Institutos de Paterna,undefined
[4] Universidade Técnica de Lisboa,undefined
[5] Laboratoire de Physique Théorique,undefined
[6] CNRS — UMR 8627,undefined
来源
Journal of High Energy Physics | / 2012卷
关键词
Higgs Physics; Rare Decays; Neutrino Physics; Supersymmetric Standard Model;
D O I
暂无
中图分类号
学科分类号
摘要
Motivated by the ATLAS and CMS discovery of a Higgs-like boson with a mass around 125 GeV, and by the need of explaining neutrino masses, we analyse the three canonical SUSY versions of the seesaw mechanism (type I, II and III) with CMSSM boundary conditions. In type II and III cases, SUSY particles are lighter than in the CMSSM (or the constrained type I seesaw), for the same set of input parameters at the universality scale. Thus, to explain \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$ {m_{{{h^0}}}}\simeq 125 $\end{document} GeV at low energies, one is forced into regions of parameter space with very large values of m0, M1/2 or A0. We compare the squark and gluino masses allowed by the ATLAS and CMS ranges for \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$ {m_{{{h^{{^0}}}}}} $\end{document} (extracted from the 2011-2012 data), and discuss the possibility of distinguishing seesaw models in view of future results on SUSY searches. In particular, we briefly comment on the discovery potential of LHC upgrades, for squark/gluino mass ranges required by present Higgs mass constraints. A discrimination between different seesaw models cannot rely on the Higgs mass data alone, therefore we also take into account the MEG upper limit on BR(μ → eγ) and show that, in some cases, this may help to restrict the SUSY parameter space, as well as to set complementary limits on the seesaw scale.
引用
收藏
相关论文
共 312 条
[11]  
Sanford D(2012)Constraints on the MSSM from the Higgs sector: a pMSSM study of Higgs searches, JHEP 03 014-undefined
[12]  
Heinemeyer S(2012) and dark matter direct detection JHEP 03 044-undefined
[13]  
Stal O(2012)Implications of a 125 GeV Higgs for the MSSM and low-scale SUSY breaking Eur. Phys. J. C 72 2020-undefined
[14]  
Weiglein G(2012)Extra matters decree the relatively heavy Higgs of mass about 125 GeV in the supersymmetric model Phys. Rev. D 85 075001-undefined
[15]  
Arbey A(2012)A 125 GeV SM-like Higgs in the MSSM and the γγ rate JHEP 05 061-undefined
[16]  
Battaglia M(2012)A Higgs boson near 125 GeV with enhanced di-photon signal in the NMSSM Phys. Lett. B 710 665-undefined
[17]  
Djouadi A(2012)Higgs and supersymmetry JHEP 02 144-undefined
[18]  
Mahmoudi F(2012)Higgs boson mass predictions in SUGRA unification, recent LHC-7 results and dark matter Phys. Lett. B 710 454-undefined
[19]  
Quevillon J(2012)Implications of the 125 GeV Higgs boson for scalar dark matter and for the CMSSM phenomenology Nucl. Phys. B 862 710-undefined
[20]  
Arbey A(2012)Current experimental constraints on the lightest Higgs boson mass in the constrained MSSM Phys. Lett. B 711 353-undefined