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Magnetic dark matter for the X-ray line at 3.55 keV

机译:X射线线在3.55 keV时的磁性暗物质

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We consider a decaying magnetic dark matter explaining the X-ray line at 3.55 ? keV shown recently from XMM-Newton observations. We introduce two singlet Majorana fermions that have almost degenerate masses and fermion–portal couplings with a charged scalar of weak scale mass. In our model, an approximate Z 2 symmetry gives rise to a tiny transition magnetic moment between the Majorana fermions at one loop. The heavier Majorana fermion becomes a thermal dark matter due to the sizable fermion–portal coupling to the SM charged fermions. We find the parameter space for the masses of dark matter and charged scalar and their couplings, being consistent with both the relic density and the X-ray line. Various phenomenological constraints on the model are also discussed.
机译:我们考虑一个衰变的磁性暗物质,解释了X射线在3.55? keV最近来自XMM-Newton观测结果显示。我们介绍了两个单态马略拉费米子,它们的质量几乎都退化了,并且费米子与门之间的耦合带有弱尺度质量的带电标量。在我们的模型中,近似的Z 2对称性在一个循环中在马里亚纳费米子之间产生了一个微小的过渡磁矩。由于相当大的费米子-门户与SM带电费米子的耦合,较重的马洛拉纳费米子变成热暗物质。我们发现暗物质和带电标量及其耦合的参数空间与文物密度和X射线线一致。还讨论了模型的各种现象学约束。

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