论文标题
$κ$ - 模型，是暗物质的最小模型替代品。应用于银河旋转问题
The $κ$-model, a minimal model alternative to dark matter. Application to the galactic rotation problem
论文作者
论文摘要
在星系中给定位置处的速度，加速度和重力场强度的测定可能会出乎意料地与观察者的环境（例如，星系中的局部平均质量密度）实现。此处通过一项有关螺旋星系旋转的研究说明了这一想法，并由不对称距离概念支持。该建议在天体物理学领域是新的（在下面，称为\ k {appa} -model），可以帮助模仿修改后的牛顿动力学（MOND）理论，修改性重力（MOG）模型或其他相关模型中所见的主要效果，以消除已经建立了已经建立过的深色问题的目的。因此，从两个选择的星系示例开始，在第5节中，我们表明Mond和\ k {appa} -model之间存在等效性。特别是，在另一侧，我们具有主要的范式的投机性，即难以捉摸的暗物质，尽管有50多年的理论，实验性和观察性努力，但其特性始终保持不确定。
The determination of the velocities, accelerations and the gravitational field intensity at a given location in a galaxy could potentially be achieved in an unexpected manner with the environment of the observer, for instance, the local mean mass density in the galaxy. This idea, mathematically supported by the asymmetric distance concept, is illustrated here by a study regarding the rotation of spiral galaxies. This suggestion is new in the astrophysics field (in the following, it is called the \k{appa}-model) and could help to mimic the main effects seen in modified Newtonian dynamics (MOND) theory, modified gravity (MOG) models, or other related models built with the aim of eliminating dark matter that are already well-established theories. Thus, starting from two selected examples of galaxies, in section 5, we show that there is an equivalence between MOND and the \k{appa}-model. In particular, on the opposite side, we have the speculative nature of the dominant paradigm, the elusive dark matter, a matter whose properties always remain undefined despite intense theoretical, experimental and observational efforts for over 50 years.
