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从Ｄｉｒａｃ四分量旋量方程出发，经广义Ｔｏｒｔｏｉｓｅ坐标变换，直接导出含有双荷子球对称黑洞的视界面位置。在推导视界温度的过程中，取消了传统的工作假设，并最终获得了Ｄｉｒａｃ粒子的Ｈａｗｋ－ｉｎｇ热谱公式．
Starting from the Dirac four-component spin equation, the generalized Tortoise coordinate transformation is used to directly derive the position of the visual interface containing the double-charge spherical symmetric black hole. In the process of deriving the horizon temperature, the traditional working hypothesis was canceled and finally the Hawk-ing thermogram of Dirac particles was obtained.