在加速直线运动时空中,采用新的Tortoise坐标变换将Dirac方程在黑洞视界面附近化成了典型的波动方程,得到在视界面附近带Dirac粒子的Hawking辐射温度,导出了Hawk-ing热辐射谱.
In rectilinearly nonuniformly accelerating space time, Dirac particles is tured into classical wave equation near the event horizon of black hole wite the change of new Tortoise coordinate system. The authors educe the formulation of Hawking thermal spectrum successfully and obtain the Hawking radiation temperature of Dirac particles near the event horizon.