Solving the dark-matter problem through dynamic interactions
Solving the dark-matter problem through dynamic interactions
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DOI：
10.1007/s11467-015-0514-9
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发表时间：
2015-06
影响因子：
7.5
通讯作者：
W. Hofer
中科院分区：
文献类型：
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作者：
W. Hofer
由于大型强子对撞机的升级及其对暗物质研究的贡献，人们对暗物质重新产生了兴趣，重新评估整个问题是及时的。考虑暗物质是调和星系外部区域物质速度与观测到的星系质量之间差异的一种方法。到目前为止，还没有确定暗物质的可靠候选者。在这里，我们开发了一个模型，通过类似于磁场的旋转物体之间的旋转和相互作用以及与移动电荷的相互作用来解释观测。这些场的大小可以用一个基本常数来描述，其量级为10− 41 kg −1。在太阳系中可以观察到同样的相互作用，它们导致行星轨道的微小变化。
Owing to the renewed interest in dark matter after the upgrade of the large hadron collider and its dedication to dark-matter research, it is timely to reassess the whole problem. Considering dark matter is one way to reconcile the discrepancy between the velocity of matter in the outer regions of galaxies and the observed galactic mass. Thus far, no credible candidate for dark matter has been identified. Here, we develop a model accounting for observations by rotations and interactions between rotating objects analogous to magnetic fields and interactions with moving charges. The magnitude of these fields is described by a fundamental constant on the order of 10−41kg−1. The same interactions can be observed in the solar system, where they lead to small changes in planetary orbits.