TY - JOUR
T1 - Exploration of the MSSM with non-universal Higgs masses
AU - Ellis, John
AU - Falk, Toby
AU - Olive, Keith A.
AU - Santoso, Yudi
PY - 2003/3/3
Y1 - 2003/3/3
N2 - We explore the parameter space of the minimal supersymmetric extension of the Standard Model (MSSM), allowing the soft supersymmetry-breaking masses of the Higgs multiplets, m 1 , 2 , to be non-universal (NUHM). Compared with the constrained MSSM(CMSSM) in which m 1 , 2 are required to be equal to the soft supersymmetry-breaking masses m 0 of the squark and slepton masses, the Higgs mixing parameter μ and the pseudoscalar Higgs mass m A , which are calculated in the CMSSM, are free in the NUHM model. We incorporate accelerator and dark matter constraints in determining allowed regions of the (μ,m A ), (μ,M 2 ) and (m 1 /2,m 0 ) planes for selected choices of the other NUHM parameters. In the examples studied, we find that the LSP mass cannot be reduced far below its limit in the CMSSM,whereas m A may be as small as allowed by LEP for large tan β. We present in Appendices A-D details of the calculations of neutralino-slepton, chargino-slepton and neutralino-sneutrino coannihilation needed in our exploration of the NUHM.
AB - We explore the parameter space of the minimal supersymmetric extension of the Standard Model (MSSM), allowing the soft supersymmetry-breaking masses of the Higgs multiplets, m 1 , 2 , to be non-universal (NUHM). Compared with the constrained MSSM(CMSSM) in which m 1 , 2 are required to be equal to the soft supersymmetry-breaking masses m 0 of the squark and slepton masses, the Higgs mixing parameter μ and the pseudoscalar Higgs mass m A , which are calculated in the CMSSM, are free in the NUHM model. We incorporate accelerator and dark matter constraints in determining allowed regions of the (μ,m A ), (μ,M 2 ) and (m 1 /2,m 0 ) planes for selected choices of the other NUHM parameters. In the examples studied, we find that the LSP mass cannot be reduced far below its limit in the CMSSM,whereas m A may be as small as allowed by LEP for large tan β. We present in Appendices A-D details of the calculations of neutralino-slepton, chargino-slepton and neutralino-sneutrino coannihilation needed in our exploration of the NUHM.
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U2 - 10.1016/S0550-3213(02)01144-6
DO - 10.1016/S0550-3213(02)01144-6
M3 - Article
AN - SCOPUS:0037416938
SN - 0550-3213
VL - 652
SP - 259
EP - 347
JO - Nuclear Physics B
JF - Nuclear Physics B
ER -