论文标题
关于Schwarzschild Spacetime的能量，并具有后牛顿后近似
On the energy of Schwarzschild spacetime with the post-Newtonian approximation
论文作者
论文摘要
随着牛顿后的近似，获得了温伯格处方中施瓦茨柴尔兹时空的能量。第一个牛顿后近似值$ e^{（1）} = m $的能量给出了牛顿史施瓦茨柴尔德时空的处理。但是，对于第二个牛顿后近似，表明$ e^{（1）} $添加了额外的术语$ e^{（2）} $，其中由配置中存储的能量$ e _ {\ rm config} $组成，在重力场$ e e _ {\ rm field} $中。以及表面积分的术语。这些额外的术语为牛顿后的牛顿治疗提供了更正。
With the post-Newtonian approxination, the energy of Schwarzschild spacetime in the Weinberg prescription is obtained. The energy for the first post-Newtonian approximation $E^{(1)} = m$ gives the Newtonian treatment of Schwarzschild spacetime. However, for the second post-Newtonian approximation, the erergy is shown that $E^{(1)}$ adds extra terms $E^{(2)}$ which consist of the energy stored in the configuration $E_{\rm config}$, in the gravitational field $E_{\rm field}$. and a term of surface integral. These extra terms gives post-Newtonian corrections to the Newtonian treatment.
