论文标题
分形引力
Fractal Gravitation
论文作者
论文摘要
考虑到{$ \ 10^6 $}星周围{barycenter，}的Gaia数据，我们以银河系的方式估算了不同区域的分形维度。然后，我们使用这些分形尺寸来计算介质作为连续分形的重力电势。最后，{我们使用引力潜力来推断}圆速度{并以银河系的方式调整}旋转曲线。 {为此，}我们使用两个数值模型，第一个考虑均匀密度，第二个考虑凸起和磁盘更现实。在这些模型中，我们都不考虑暗物质。我们研究了他们的有效性，将它们与银河系中的循环速度数据进行了比较。
Considering the GAIA data for {$\approx 10^6$} stars around the {barycenter,} we estimate the fractal dimension for different regions in the Milky Way. Then we use those fractal dimensions to calculate the gravitational potential considering the medium as a continuous fractal. Finally, {we use the gravitational potential to infer} the circular velocity {and adjust} rotation curves in the Milky Way. {For this,} we use two numerical models, the first considering uniform density and a second more realistic of a bulge and a disk. In none of these models we consider dark matter. We study their validity comparing them with circular speed data from the Milky Way.
