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arXiv 0909.4181hep-ph
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Gamma ray线路:关于SUSY,它们会告诉我们什么?

Gamma ray lines: what will they tell us about SUSY?

Carlos E. Yaguna

摘要:

中性子暗物质可以通过观测湮灭过程XX-->gg和XX-->gZ的γ射线线间接探测到。在本文中,我们研究的影响,这两条线的观察可能有超对称参数空间的确定。在最小超引力框架内,我们发现,独立于银河系中的暗物质分布,这样的观测本身就可以区分共湮灭区、漏斗区和焦点区。因此,可以导出对msugra参数的几个限制。在一个更一般的MSSM的情况下,我们表明,伽马射线线的观测可能会被用来区分一个比诺,一个维诺,和希格斯诺类中性伴子,宇宙学和模型的超对称性破缺的重要后果。因此,对伽马射线线的探测不仅将提供一个明确无误的暗物质特征,还将为确定超对称参数开辟一条新的道路。

英文摘要:

Neutralino dark matter can be indirectly detected by observing the gamma ray lines from the annihilation processes XX-->gg and XX-->gZ. In this paper we study the implications that the observation of these two lines could have for the determination of the supersymmetric parameter space. Within the minimal supergravity framework, we find that, independently of the dark matter distribution in the Galaxy, such observations by themselves would allow to differentiate between the coannihilation region, the funnel region, and the focus point region. As a result, several restrictions on the msugra parameters can be derived. Within a more general MSSM scenario, we show that the observation of gamma-ray lines might be used to discriminate between a bino-, a wino-, and a higgsino-like neutralino, with important consequences for cosmology and for models of supersymmetry breaking. The detection of the gamma ray lines, therefore, will not only provide an unmistakable signature of dark matter, it will also open a new road toward the determination of supersymmetric parameters.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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