In this paper we leave the neighborhood of the singularity at the origin andturn to the singularity at the horizon. Using nonlinear superdistributionalgeometry and supergeneralized functions it seems possible to show that thehorizon singularity is not only a coordinate singularity without leavingSchwarzschild coordinates. However the Tolman formula for the total energy $E$of a static and asymptotically flat spacetime,gives $E=mc^2$, as it should be.New class Colombeau solutions to Einstein field equations is obtained.New classColombeau solutions to Einstein field equations is obtained. The vacuum energydensity of free scalar quantum field $F$ with a distributional backgroundspacetime also is considered.
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机译:在本文中,我们在原点离开奇点的邻域,然后在地平线上转向奇点。使用非线性超分布几何和超广义函数,似乎有可能表明,在不离开Schwarzschild坐标的情况下,水平奇异不仅是坐标奇异。然而,静态和渐近平坦时空的总能量$ E $的Tolman公式应给出$ E = mc ^ 2 $。获得了爱因斯坦场方程的新类Colombeau解。得到方程式。还考虑了具有分布背景时空的自由标量量子场$ F $的真空能量密度。
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