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Multiple ultralight axionic wave dark matter and astronomical structures
Physics of the Dark Universe ( IF 5.0 ) Pub Date : 2020-06-17 , DOI: 10.1016/j.dark.2020.100636
Hoang Nhan Luu , S.-H. Henry Tye , Tom Broadhurst

An ultralight scalar boson with mass m11022eV is gaining credence as a Dark Matter (DM) candidate that explains the dark cores of dwarf galaxies as soliton waves. Such a boson is naturally interpreted as an axion generic in String Theory, with multiple light axions predicted in this context. We examine the possibility of soliton structures over a wide range of scales, accounting for galaxy core masses and the common presence of nuclear star clusters. We present a diagnostic soliton core mass–radius plot that provides a global view, indicating the existence of an additional axion with mass m21020eV, with the possibility of a third axion with mass m30.5×1018eV. We also argue that the relative mass densities measured for these axions are consistent with their cosmological production via the mis-alignment mechanism.



中文翻译:

多个超轻质子轴波暗物质和天文结构

超轻质标量玻色子 1个1个0-22电子伏特作为暗物质(DM)候选者而获得了信任,该候选者将矮星系的暗核解释为孤子波。这样的玻色子自然被解释为弦理论中的通用轴,在这种情况下可以预测出多个轻轴。我们检查了范围广泛的尺度上的孤子结构的可能性,其中考虑了星系核心质量和核星团的普遍存在。我们提出了诊断孤子核心质量半径图,该图提供了一个整体视图,表明存在附加的质量轴21个0-20电子伏特,有可能发生第三次弥撒 305×1个0-18岁电子伏特。我们还认为,针对这些轴的相对质量密度通过失准机制与它们的宇宙生产相一致。

更新日期:2020-06-17
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