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利用广义不确定关系修正的态密度方程并采用WKB近似方法, 计算了Gibbons-Maeda黑洞时空中标量场的统计力学熵. 所得的统计力学熵与该黑洞的视界面积成正比, 与Brick-Wall方法所得的结果相同, 但不需要取任何截断就能避免Brick-Wall方法的发散问题.
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关键词:
- 广义不确定关系 /
- Gibbons-Maeda黑洞 /
- 态密度 /
- 统计力学熵
Statistical entropy of scalar field outside Gibbons-Maeda black hole is computed by the equation of state density corrected by the generalized uncertainty principle and by WKB approximation method. The result shows that the black hole entropy is proportional to its horizon area, which is the same as that given by Brick-Wall method. The difference from the Brick-Wall method is that the present result is convergent without any cutoff.-
Keywords:
- generalized uncertainty principle /
- Gibbons-Maeda black hole /
- state density /
- statistical entropy
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