【摘要】 研究了匀加速直线运动的稳态Ｋｅｒｒ黑洞的热性质，发现它的Ｒｉｎｄｌｅｒ视界面的Ｕｎｒｕｈ温度和它的事件视界的Ｈａｗｋｉｎｇ温度都不再是常数，而是的函数，得到了黑洞表面各点的温度．当它的Ｒｉｎｄｌｅｒ视界与事件视界发生碰撞时，在接触点温度都变为零；而在黑洞视界的另一相反极点处Ｈａｗｋｉｎｇ温度将增大更多还原

【Abstract】 Thermal properties of a uniformly accelerating rectilinear stationary Kerr blackhole are studied. It is discoveral that both the Unruh temperature of the Rindler horizon andthe Hawking temperature of the event horizon are no longer constant. They are funtions depending on 0. Furthermore, the temperature of every point on the black hole surface can beobtained. When the event horizon collides with the Rindler horizon,the temperature at thecontact point will reduce to zero.But, at the opposite pole of the ever horizon of black hole,the Hawking temperatUre will increase.更多还原