摘要
在本文中我们得到了慢速运动中两个球对称非旋转天体在辐射作用力影响下的运动方程。此方程相对论改正达到了(v/c)~2、(v/c)~4、(v/c)~5量级。运动方程只依赖于相对论质量,而与天体的内部结构和致密度无直接关系。这意味着运动方程可以应用于象中子星和黑洞一类具有强内引力的天体。
In the slow speed motion approximation, we have obtained the equations of motion for two spherically-symmetric,non rotating bodies with the radiative force.The equations include relativistic corrections of order (v/c)~2,(v/c)~4, and(v/c)~5 to the newtonian corrections. It is shown that the equations depend on the relativistic mass, regardless of the internal structrre and degree of compactness. This means that the equations can be applied to bodies with strong internal gravity, such as neutron stars and black holes.
基金
中科院紫台小行星基金
