$U(1)_{\chi}$、Seesaw暗物质和希格斯衰变

Q2 Physics and Astronomy Letters in High Energy Physics Pub Date : 2018-10-15 DOI:10.31526/LHEP.1.2019.103
E. Ma
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引用次数: 6

摘要

最近有人指出,暗物质的基本对称性很可能是$U(1)_\chi$(从$SO(10)到SU(5)\乘以U(1。有了这一新的见解,以前的简单暗物质模型得到了重新解释,并提出了一个新的想法,即光跷跷板暗物质的存在类似于光中微子,是由标准模型希格斯玻色子的罕见衰变产生的。
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$U(1)_{\chi}$, Seesaw Dark Matter, and Higgs Decay
It has recently been pointed out that the underlying symmetry of dark matter may well be $U(1)_\chi$ (coming from $SO(10) \to SU(5) \times U(1)_\chi$) with the dark parity of any given particle determined by $(-1)^{Q_\chi+2j}$, where $Q_\chi$ is its $U(1)_\chi$ charge and $j$ its spin angular momentum. Armed with this new insight, previous simple models of dark matter are reinterpreted, and a novel idea is proposed that light seesaw dark matter exists in analogy to light neutrinos and is produced by the rare decay of the standard-model Higgs boson.
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来源期刊
Letters in High Energy Physics
Letters in High Energy Physics Physics and Astronomy-Nuclear and High Energy Physics
CiteScore
1.20
自引率
0.00%
发文量
4
审稿时长
12 weeks
期刊最新文献
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