Right-handed sneutrino as cold dark matter of the universe

Right-handed sneutrino as cold dark matter of the universe
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DOI:
10.1103/physrevd.75.065001
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发表时间:
2006-12
期刊:
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影响因子:
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通讯作者:
T. Asaka;Koji Ishiwata;T. Moroi
T. Asaka;Koji Ishiwata;T. Moroi
中科院分区:
其他
文献类型:
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作者:
T. Asaka;Koji Ishiwata;T. Moroi

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本文研究了由三个右手中微子扩展的最小超对称标准模型。假设中微子的质量是纯粹的狄拉克型,最轻的右手中微子R可以是最轻的超粒子(LSP)。我们讨论了LSP-R成为宇宙暗物质的可能性,特别关注了早期宇宙中R的产生。这项工作是基于与K. Ishiwata和T. Moroi [1,2].
We consider the minimal supersymmetric standard model (MSSM) extended by three right-handed neutrinos. Assuming that neutrino masses are purely Dirac-type, the lightest right-handed sneutrino R can be the lightest superparticle (LSP). We discuss the possibility that the LSP R becomes dark matter of the universe, paying attention to the production of R in the early universe. This work is based on collaboration with K. Ishiwata and T. Moroi [1, 2].