As an example, the critical condition for the streaming gravity mode instability is discussed in a weak gravitational field.
作为一个例子,还讨论了弱重力场情况下激发流动重力模不稳定性的临界条件。
Besides that, we presents the gravitational wave energy density under the weak field situation and gives the x - y plane numerical calculation to curvature scalar R and energy density .
还有计算了在弱场条件近似下引力驻波的能量密度,并给出曲率标量R和能量密度平面的数值计算。
In chapter two, it explains gravitational radiation, especially the linear solution in gravitational field. That means it gives explanation to weak field.
在第二章中,介绍了引力辐射,主要是对引力场的线性化求解,即弱场近似作了介绍。
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