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arXiv 0704.3446hep-phastro-phhep-ex
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无GUT超对称破缺的唯象

Phenomenology of GUT-less Supersymmetry Breaking

John Ellis, Keith A. Olive, Pearl Sandick

摘要:

我们研究的模型中,超对称性破缺出现在一个中间尺度,M_{in},低于大统一理论的规模。我们假设MSSM的软超对称破缺参数在M_{in}是普适的,并分析了当M_{in}从GUT尺度缩减时,宇宙学和对撞机实验对参数空间允许区域的约束形态。我们提出了单独的分析(m_{1/2},m_0)平面的tan(β)=10和tan(β)=50,以及非零三线性耦合,A_0的讨论。在微扰-中介模型中,我们也在这里讨论了高根诺质量和标量质量在大统一理论尺度下似乎是普遍存在的具体情况。我们要求最轻的中性伴子是LSP,并且残余中性伴子密度与WMAP和其他观测的测量值不冲突。在中等的M_{in}值下,我们发现(m_{1/2},m_0)平面的允许区域被电弱对称性破缺的要求压缩,最轻的中性伴子是LSP,而对残余密度的约束不那么严格。在非常低的M_{in},电弱真空条件成为主要的约束,和天体物理冷暗物质的第二个来源将是必要的,以解释几乎所有的软超对称性破缺参数和tan(β)值的测量遗迹密度。我们计算中性子核子截面可行的方案,并将它们与目前和预测的直接暗物质搜索的限制。

英文摘要:

We study models in which supersymmetry breaking appears at an intermediate scale, M_{in}, below the GUT scale. We assume that the soft supersymmetry-breaking parameters of the MSSM are universal at M_{in}, and analyze the morphology of the constraints from cosmology and collider experiments on the allowed regions of parameter space as M_{in} is reduced from the GUT scale. We present separate analyses of the (m_{1/2},m_0) planes for tan(beta)=10 and tan(beta)=50, as well as a discussion of non-zero trilinear couplings, A_0. Specific scenarios where the gaugino and scalar masses appear to be universal below the GUT scale have been found in mirage-mediation models, which we also address here. We demand that the lightest neutralino be the LSP, and that the relic neutralino density not conflict with measurements by WMAP and other observations. At moderate values of M_{in}, we find that the allowed regions of the (m_{1/2},m_0) plane are squeezed by the requirements of electroweak symmetry breaking and that the lightest neutralino be the LSP, whereas the constraint on the relic density is less severe. At very low M_{in}, the electroweak vacuum conditions become the dominant constraint, and a secondary source of astrophysical cold dark matter would be necessary to explain the measured relic density for nearly all values of the soft SUSY-breaking parameters and tan(beta). We calculate the neutralino-nucleon cross sections for viable scenarios and compare them with the present and projected limits from direct dark matter searches.

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