E-Wimps

E-Wimps
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电子懦夫

DOI:
10.1063/1.2149672
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发表时间:
2005
影响因子:
5.4
通讯作者:
L. Roszkowski
L. Roszkowski
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
Ki;L. Roszkowski

文献摘要

被引文献

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极弱相互作用大质量粒子(e - wimp)是宇宙中冷暗物质的有趣候选者。我们回顾了两个良好激发的e - wimp,一个轴子和一个引力子,并指出了它们在宇宙学和现象学上的异同,后者可以让人们在LHC寻找超对称时区分它们。
Extremely weakly interacting massive particles (E-WIMPs) are intriguing candidates for cold dark matter in the Universe. We review two well motivated E-WIMPs, an axino and a gravitino, and point out their cosmological and phenomenological similarities and differences, the latter of which may allow one to distinguishing them in LHC searches for supersymmetry.