Ellis John, Evans Jason L, Luo Feng, Nagata Natsumi, Olive Keith A, Sandick Pearl
Theoretical Physics and Cosmology Group, Department of Physics, King's College London, Strand, London, WC2R 2LS UK ; TH Division, Physics Department, CERN, 1211 Geneva 23, Switzerland.
William I. Fine Theoretical Physics Institute, School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 USA.
Eur Phys J C Part Fields. 2016;76:8. doi: 10.1140/epjc/s10052-015-3842-6. Epub 2016 Jan 5.
We consider two potential non-accelerator signatures of generalizations of the well-studied constrained minimal supersymmetric standard model (CMSSM). In one generalization, the universality constraints on soft supersymmetry-breaking parameters are applied at some input scale [Formula: see text] the grand unification (GUT) scale [Formula: see text], a scenario referred to as 'sub-GUT'. The other generalization we consider is to retain GUT-scale universality for the squark and slepton masses, but to relax universality for the soft supersymmetry-breaking contributions to the masses of the Higgs doublets. As with other CMSSM-like models, the measured Higgs mass requires supersymmetric particle masses near or beyond the TeV scale. Because of these rather heavy sparticle masses, the embedding of these CMSSM-like models in a minimal SU(5) model of grand unification can yield a proton lifetime consistent with current experimental limits, and may be accessible in existing and future proton decay experiments. Another possible signature of these CMSSM-like models is direct detection of supersymmetric dark matter. The direct dark matter scattering rate is typically below the reach of the LUX-ZEPLIN (LZ) experiment if [Formula: see text] is close to [Formula: see text], but it may lie within its reach if [Formula: see text] GeV. Likewise, generalizing the CMSSM to allow non-universal supersymmetry-breaking contributions to the Higgs offers extensive possibilities for models within reach of the LZ experiment that have long proton lifetimes.
我们考虑了经过充分研究的约束最小超对称标准模型(CMSSM)推广中的两种潜在非加速器特征。在一种推广中,对软超对称破缺参数的通用性约束应用于某个输入尺度(大统一(GUT)尺度),这种情形被称为“亚GUT”。我们考虑的另一种推广是,对于夸克和轻子质量保留GUT尺度的通用性,但放宽对希格斯二重态质量的软超对称破缺贡献的通用性。与其他类似CMSSM的模型一样,测得的希格斯质量要求超对称粒子质量接近或超过 TeV 尺度。由于这些超对称粒子质量相当大,将这些类似CMSSM的模型嵌入最小 SU(5) 大统一模型中可以产生与当前实验限制相符的质子寿命,并且可能在现有的和未来的质子衰变实验中被探测到。这些类似CMSSM的模型的另一个可能特征是直接探测超对称暗物质。如果 接近 ,直接暗物质散射率通常低于LUX-ZEPLIN(LZ)实验的探测范围,但如果 GeV,则可能在其探测范围内。同样,将CMSSM推广以允许对希格斯有非通用的超对称破缺贡献,为具有长质子寿命且在LZ实验探测范围内的模型提供了广泛的可能性。