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arXiv 0812.1859hep-ph
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MSSM暴胀子:SUSY暗物质和LHC

MSSM inflaton: SUSY dark matter and LHC

A. Mazumdar

摘要:

在这次演讲中,我们将讨论如何将暴胀嵌入到标准模型的最小扩展中,其中暴胀子携带标准模型电荷。为了解释宇宙微波背景辐射的温度各向异性,不需要引入一个特定的标量场,所有的成分都存在于一个最小的超对称标准模型中。暴胀子的性质第一次可以直接与粒子唯象学、暗物质和标准模型的重子联系起来。

英文摘要:

In this talk we will discuss how inflation can be embedded within a minimal extension of the Standard Model where the inflaton carries the Standard Model charges. There is no need of an ad-hoc scalar field to be introduced in order to explain the temperature anisotropy of the cosmic microwave background radiation, all the ingredients are present within a minimal supersymmetric Standard Model. For the first time inflaton properties can be directly linked to the particle phenomenology, dark matter, and the baryons of the Standard Model.

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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