用视界表面引力的定义,即相对于视界静止质点的固有加速度和红移因子的乘积在质点趋于视界时的极限、Klein-Gordon方程与Hamilton-Jacobi方程3种方法研究了稳态Kerr-Newman-Kasuya黑洞视界表面引力.其结果表明黑洞的视界表面引力与黑洞所带电荷、磁荷和角动量等因素有关.
Three methods are used to study the horizon surface gravitation of Kerr-Newman-Kasuya Black Hole, which are definition method, i. e. the product' limit which is made by reversely slack particles' underlying acceleration for the event horizon and the Einstein shift, Klein-Gordon equation and Hamilton-Jacobi equation. The result shows that the horizon surface gravitation of this black hole is related to charges, magnetizations, angle momentum and other factors of this black hole.