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arXiv 0909.2484hep-ph
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超对称跷跷板模型中电弱对称性和中性伴子暗物质辐射破缺的阈值修正

Threshold corrections to the radiative breaking of electroweak symmetry and neutralino dark matter in supersymmetric seesaw model

Sin Kyu Kang, Akina Kato, Takuya Morozumi, Norimi Yokozaki

摘要:

在超对称I型跷跷板模型中研究了中性伴子暗物质的辐射电弱对称破缺和剩余丰度。在该模型中,由于重单重中微子环对Higgs双线性项的阈值修正,使得上型Higgs的软超对称破缺(SSB)质量在跷跷板尺度上发生位移,从而影响了Higgs势的极小化条件.我们表明,所需的微调之间的Higgsino质量参数μ和SSB的质量向上型希格斯粒子可能会减少在电弱尺度,由于阈值修正。我们还介绍了如何μ参数依赖于重单重sneutrinos的SSB B参数。由于中性伴子暗物质的性质对μ的大小非常敏感,我们讨论了SSB B参数对中性伴子暗物质残余丰度的影响。取几百TeV量级的单边带B参数,可以正确地获得所需的中性伴子暗物质残余丰度。在这种情况下,暗物质是比诺和希格斯诺的混合物,条件是高吉诺质量在大统一尺度下是普适的。

英文摘要:

We study the radiative electroweak symmetry breaking and the relic abundance of neutralino dark matter in the supersymmetric type I seesaw model. In this model, there exist threshold corrections to Higgs bilinear terms coming from heavy singlet sneutrino loops, which make the soft supersymmetry breaking (SSB) mass for up-type Higgs shift at the seesaw scale and thus a minimization condition for the Higgs potential is affected. We show that the required fine-tuning between the Higgsino mass parameter mu and the SSB mass for up-type Higgs may be reduced at the electroweak scale, due to the threshold corrections. We also present how the parameter mu depends on the SSB B-parameter for heavy singlet sneutrinos. Since the property of neutralino dark matter is quite sensitive to the size of mu, we discuss how the relic abundance of neutralino dark matter is affected by the SSB B-parameter. Taking the SSB B-parameter of order of a few hundreds TeV, the required relic abundance of neutralino dark matter can be correctly achieved. In this case, dark matter is a mixture of bino and Higgsino, under the condition that gaugino masses are universal at the grand unification scale.

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