论文标题
磁盘星系旋转曲线的相对论校正
Relativistic corrections to the rotation curves of disk galaxies
论文作者
论文摘要
我们提出了一种研究大量大量产生的相对论效应的方法。该方法是非扰动的，并采用了平均场近似和重力镜头。使用此方法和磁盘星系的基本模型，我们发现对磁盘星系旋转曲线的相对论校正在大银河半径上是显着的。该模型预测了推断的银河系深质量与银河盘厚度之间的密切相关性，我们使用两组单独的观测数据进行了验证。
We present a method to investigate relativistic effects arising from large masses. The method is non-perturbative and employs a mean-field approximation and gravitational lensing. Using this method and a basic model of disk galaxy, we find that relativistic corrections to the rotation curves of disk galaxies are significant at large galactic radii. The model predicts a strong correlation between the inferred galactic dark mass and the galactic disk thickness, which we verified using two separate sets of observational data.
