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arXiv 2303.13643hep-phastro-ph.HE
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GeV能标以下的多极矢量暗物质

Multipole vector dark matter below the GeV-scale

Xiaoyong Chu, Junji Hisano, Alejandro Ibarra, Jui-Lin Kuo, Josef Pradler

AI总结:

研究GeV能标以下电中性复矢量粒子通过高维形状因子与光子耦合构成暗物质,推导了天体物理约束,结合直接/间接探测与宇宙学限制,计算遗迹密度并分析参数空间自然性。

摘要:

我们考虑GeV质量标度以下电中性复矢量粒子$V$,从低能视角看,它们通过高维度形状因子相互作用与光子耦合。我们通过考虑太阳、水平分支星和红巨星以及SN1987A中矢量粒子对产生导致的异常能量损失,推导了相应的天体物理约束。在暗态$V$构成暗物质的假设下,这些界限由直接和间接探测以及宇宙学限制加以补充。我们还计算了来自freeze-out和freeze-in机制的遗迹密度。基于实现所考虑有效耦合的UV-complete模型,我们还讨论了受约束参数空间的自然性,并对$V$的零质量极限进行了分析。

英文摘要:

We consider electrically neutral complex vector particles $V$ below the GeV mass scale that, from a low energy perspective, couple to the photon via higher dimensional form factor interactions. We derive ensuing astrophysical constraints by considering the anomalous energy loss from the Sun, Horizontal Branch, and Red Giant stars as well as from SN1987A that arise from vector pair-production in these environments. Under the assumption that the dark states $V$ constitute dark matter, the bounds are then complemented by direct and indirect detection as well as cosmological limits. The relic density from freeze-out and freeze-in mechanisms is also computed. On the basis of a UV-complete model that realizes the considered effective couplings, we also discuss the naturalness of the constrained parameter space, and provide an analysis of the zero mass limit of $V$.

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